ANCHORS:Resetting CIAO and Parameters
ANCHORS: wav_rec_blo_expmap.sh output
Reading config file /data/ANCHORS/YAXX/bin/yaxx-0.908-linux/yaxx.cfg
Reading config file /data/ANCHORS/YAXX/00619/yaxx.cfg
Reading config file /data/ANCHORS/YAXX/bin/yaxx-0.908-linux/resources/Chandra/yaxx.cfg
Reading config file /data/ANCHORS/YAXX/00619/yaxx.cfg.test
Initializing CIAO environment
Successfully inited CIAO using source /soft/ciao/bin/ciao.csh
Reading object list from sample.rdb

**********************************************************************
***  Obsid=619  Srcid=1                                            ***
**********************************************************************
<2007-May-31 15:24:55> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/acis_asol1.fits
Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/acis_bpix1.fits
Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 0 719 801 SKY 3668.9292603 4275.3348389
Background Event statistics: CHIP 0 697.5 818.5 SKY 3657.5054932 4261.1052246

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=513:768,chipy=801:832]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=513:768,chipy=801:832]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=513:768,chipy=801:832] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=0]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (3668.9292603,4275.3348389)
mkarf detsubsys=ACIS-I0 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=3668.9292603 sourcepixely=4275.3348389 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src1/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	4 
   mean:	0.0076045627376 
  sigma:	0.086871936569 
    sum:	4 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
4
Running dmstat
     infile=obs619/src1/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	0 	      @:	1 
   mean:	0 
  sigma:	0 
    sum:	0 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
0
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src1/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     5.93676E+00
 powll:     converged to minimum =     4.97850E-15 at iteration =      3
 powll:    final statistic value =     4.97850E-15
    bkg_mdl_c1.factor  0     

WARNING:
   The value of bkg_mdl_c1.factor is equal to the bkg_mdl_c1.factor.min limit boundary.
   You may wish to consider changing min/max values and refitting.

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.36878E+02
 powll:     converged to minimum =     3.15303E+01 at iteration =      9
 powll:    final statistic value =     3.15303E+01
          wabs.nH  0.0001  10^22/cm^2  
            rs.kT  1.14008  keV  
            rs.norm  6.66602e-06  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of wabs.nH is equal to the wabs.nH.min limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard minimum for  wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             0.0001    -----         +0.0758428    
            rs.kT            1.14008    -----         +5.50763      
            rs.norm      6.66602e-06  -4.0177e-06     +6.84182e-06  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
WARNING: hit parameter space hard minimum for  wabs.nH 
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             0.0001    -----         +0.0787043    
            rs.kT            1.14008    -----         +5.78672      
            rs.norm      6.66602e-06  -4.02655e-06    +7.01139e-06  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 1.05061e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.69251936,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.51342737,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    4,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1525' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:25:33> *** SUCCESS for Obsid=619  Ccdid=ACIS-I0  Srcid=1

**********************************************************************
***  Obsid=619  Srcid=2                                            ***
**********************************************************************
<2007-May-31 15:25:33> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 3 803.92857143 313.5 SKY 4407.6153739 3467.0279541
Background Event statistics: CHIP 3 796.42857143 326.5 SKY 4412.2204939 3478.9637451

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=769:1024,chipy=289:320]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=769:1024,chipy=321:352]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=769:1024,chipy=289:320] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=769:1024,chipy=321:352] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=3]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (4407.6153739,3467.0279541)
mkarf detsubsys=ACIS-I3 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4407.6153739 sourcepixely=3467.0279541 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (4412.2204939,3478.9637451)
mkarf detsubsys=ACIS-I3 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=4412.2204939 sourcepixely=3478.9637451 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src2/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	36 
   mean:	0.024714828897 
  sigma:	0.1780690003 
    sum:	13 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
13
Running dmstat
     infile=obs619/src2/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	58 
   mean:	0.0038022813688 
  sigma:	0.061545300594 
    sum:	2 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
2
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src2/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     2.28025E+01
 powll:     converged to minimum =     2.25637E+01 at iteration =      3
 powll:    final statistic value =     2.25637E+01
    bkg_mdl_c1.factor  7.21262e-05     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.43065E+02
 powll:     converged to minimum =     7.66130E+01 at iteration =     19
 powll:    final statistic value =     7.66130E+01
          wabs.nH  0.375306  10^22/cm^2  
            rs.kT  0.370471  keV  
            rs.norm  8.37835e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.375306  -0.124421       +0.151129     
            rs.kT           0.370471  -0.079179       +0.0896758    
            rs.norm      8.37835e-05  -3.19733e-05    +4.30818e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
WARNING: lower projection bound not found for  wabs.nH 
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.375306  -0.375306       +0.66581      
            rs.kT           0.370471  -0.19793        +0.398115     
            rs.norm      8.37835e-05  -7.2588e-05     +0.0046415    

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 1.21191e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.58147626,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.62397423,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    12.9258840723001,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1526' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:26:37> *** SUCCESS for Obsid=619  Ccdid=ACIS-I3  Srcid=2

**********************************************************************
***  Obsid=619  Srcid=3                                            ***
**********************************************************************
<2007-May-31 15:26:37> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 475.875 673.5 SKY 4426.0553589 4580.2875977
Background Event statistics: CHIP 2 480.53846154 662.61538462 SKY 4432.3073167 4584.0362831

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=673:704]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=641:672]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=673:704] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=641:672] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (4426.0553589,4580.2875977)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4426.0553589 sourcepixely=4580.2875977 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (4432.3073167,4584.0362831)
mkarf detsubsys=ACIS-I2 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=4432.3073167 sourcepixely=4584.0362831 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src3/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	65 
   mean:	0.015209125475 
  sigma:	0.12238385505 
    sum:	8 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
8
Running dmstat
     infile=obs619/src3/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	13 
   mean:	0.0057034220532 
  sigma:	0.075305332016 
    sum:	3 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
3
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src3/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     3.01285E+01
 powll:     converged to minimum =     3.01142E+01 at iteration =      3
 powll:    final statistic value =     3.01142E+01
    bkg_mdl_c1.factor  0.000107249     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.48429E+02
 powll:     converged to minimum =     8.64537E+01 at iteration =     14
 powll:    final statistic value =     8.64537E+01
          wabs.nH  2.13816  10^22/cm^2  
            rs.kT  2.31541  keV  
            rs.norm  7.24439e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.13816  -0.860926       +1.30831      
            rs.kT            2.31541  -0.976158       +2.49766      
            rs.norm      7.24439e-05  -3.38406e-05    +4.94038e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.13816  -0.865539       +4.05093      
            rs.kT            2.31541  -0.98355        +61.6846      
            rs.norm      7.24439e-05  -5.46062e-05    +0.00202481   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 5.33441e-06 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.57872828,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.47177400,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    7.88889028006902,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1527' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:27:39> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=3

**********************************************************************
***  Obsid=619  Srcid=4                                            ***
**********************************************************************
<2007-May-31 15:27:39> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 3 244 827 SKY 4855.5657959 4079.9606323
Background Event statistics: CHIP 3 247.51428571 824.62857143 SKY 4845.1359515 4083.6137626

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=1:256,chipy=801:832]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=1:256,chipy=801:832]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=1:256,chipy=801:832] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=3]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (4855.5657959,4079.9606323)
mkarf detsubsys=ACIS-I3 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4855.5657959 sourcepixely=4079.9606323 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src4/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	35 
   mean:	0.0076045627376 
  sigma:	0.086871936569 
    sum:	4 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
4
Running dmstat
     infile=obs619/src4/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	75 
   mean:	0.028517110266 
  sigma:	0.16644483978 
    sum:	15 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
15
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src4/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.32307E+02
 powll:     converged to minimum =     1.04928E+02 at iteration =      3
 powll:    final statistic value =     1.04928E+02
    bkg_mdl_c1.factor  0.000567752     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.84721E+02
 powll:     converged to minimum =     1.37200E+02 at iteration =      8
 powll:    final statistic value =     1.37200E+02
          wabs.nH  0.1445  10^22/cm^2  
            rs.kT  1.76723  keV  
            rs.norm  8.9333e-06  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard minimum for  wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             0.1445    -----         +0.570516     
            rs.kT            1.76723    -----           -----       
            rs.norm       8.9333e-06  -5.84067e-06    +9.98465e-06  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
WARNING: hit parameter space hard minimum for  wabs.nH 
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             0.1445    -----         +2.09676      
            rs.kT            1.76723    -----           -----       
            rs.norm       8.9333e-06  -6.63012e-06    +0.000243006  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 2.87828e-06 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.51423875,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.54015060,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    3.44443170154484,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1528' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:28:13> *** SUCCESS for Obsid=619  Ccdid=ACIS-I3  Srcid=4

**********************************************************************
***  Obsid=619  Srcid=5                                            ***
**********************************************************************
<2007-May-31 15:28:13> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 3 739.25 458.5 SKY 4434.0738525 3612.7116699
Background Event statistics: CHIP 3 729.5 459.78571429 SKY 4447.1631557 3626.0898089

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=513:768,chipy=449:480]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=513:768,chipy=449:480]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=513:768,chipy=449:480] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=3]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (4434.0738525,3612.7116699)
mkarf detsubsys=ACIS-I3 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4434.0738525 sourcepixely=3612.7116699 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src5/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	273 
   mean:	0.0076045627376 
  sigma:	0.086871936569 
    sum:	4 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
4
Running dmstat
     infile=obs619/src5/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	491 
   mean:	0.0019011406844 
  sigma:	0.043560605465 
    sum:	1 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
1
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src5/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.25700E+01
 powll:     converged to minimum =     1.09474E+01 at iteration =      3
 powll:    final statistic value =     1.09474E+01
    bkg_mdl_c1.factor  3.49248e-05     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.82085E+02
 powll:     converged to minimum =     4.15394E+01 at iteration =     44
 powll:    final statistic value =     4.15394E+01
          wabs.nH  65.4107  10^22/cm^2  
            rs.kT  1.44378  keV  
            rs.norm  0.00652281  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            65.4107  -17.6092        +26.1273      
            rs.kT            1.44378  -0.303009       +0.379232     
            rs.norm       0.00652281  -0.00394148     +0.00671202   

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            65.4107  -47.2876        +66.8431      
            rs.kT            1.44378  -2.21796        +62.5562      
            rs.norm       0.00652281  -0.0064139      +53.9676      

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 4.63947e-06 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.57753795,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.60404244,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    3.96295136657504,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1529' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:29:06> *** SUCCESS for Obsid=619  Ccdid=ACIS-I3  Srcid=5

**********************************************************************
***  Obsid=619  Srcid=6                                            ***
**********************************************************************
<2007-May-31 15:29:06> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 527.5 1014 SKY 4555.3205566 4241.2332764
Background Event statistics: CHIP 3 502 1007.25 SKY 4550.8875732 4240.0601807

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=513:768,chipy=993:1024]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=257:512,chipy=993:1024]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=513:768,chipy=993:1024] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=257:512,chipy=993:1024] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (4555.3205566,4241.2332764)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4555.3205566 sourcepixely=4241.2332764 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (4550.8875732,4240.0601807)
mkarf detsubsys=ACIS-I3 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=4550.8875732 sourcepixely=4240.0601807 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
*** WARNING: The ARF was computed to be zero at all the specified energies.
             This is probably due to an incorrect source position, or to an
             improperly selected detector.  Check your parameters carefully!
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src6/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	138 
   mean:	0.0076045627376 
  sigma:	0.086871936569 
    sum:	4 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
4
Running dmstat
     infile=obs619/src6/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	402 
   mean:	0.0019011406844 
  sigma:	0.043560605465 
    sum:	1 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
1
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src6/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.28969E+01
 powll:     converged to minimum =     1.28399E+01 at iteration =      3
 powll:    final statistic value =     1.28399E+01
    bkg_mdl_c1.factor  7.94844e-05     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.04646E+02
 powll:     converged to minimum =     4.37284E+01 at iteration =     39
 powll:    final statistic value =     4.37284E+01
          wabs.nH  14.8961  10^22/cm^2  
            rs.kT  0.657067  keV  
            rs.norm  0.0126881  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs.norm is equal to the rs.norm.max limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            14.8961  -3.99199        +6.22983      
            rs.kT           0.657067  -0.12051        +0.131759     
            rs.norm        0.0126881  -0.00757729     +0.013459     

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            14.8961  -29.4517        +53.1135      
            rs.kT           0.657067  -0.882679       +2.06537      
            rs.norm        0.0126881  -0.0125577      +492.558      

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 6.20481e-06 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.55935958,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.51814033,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    3.96295569371903,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1530' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:30:15> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=6

**********************************************************************
***  Obsid=619  Srcid=7                                            ***
**********************************************************************
<2007-May-31 15:30:15> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 0 918.66666667 306.77777778 SKY 3769.3727756 4812.0343967
Background Event statistics: CHIP 0 927.40540541 299.72972973 SKY 3776.1329973 4817.2609401

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=769:1024,chipy=289:320]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=769:1024,chipy=289:320]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=769:1024,chipy=289:320] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=0]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (3769.3727756,4812.0343967)
mkarf detsubsys=ACIS-I0 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=3769.3727756 sourcepixely=4812.0343967 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src7/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	72 
   mean:	0.01711026616 
  sigma:	0.1296823232 
    sum:	9 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
9
Running dmstat
     infile=obs619/src7/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	5 
   mean:	0.024714828897 
  sigma:	0.1552546493 
    sum:	13 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
13
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src7/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.20936E+02
 powll:     converged to minimum =     1.00393E+02 at iteration =      3
 powll:    final statistic value =     1.00393E+02
    bkg_mdl_c1.factor  0.000488024     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.75220E+02
 powll:     converged to minimum =     1.65062E+02 at iteration =     19
 powll:    final statistic value =     1.65062E+02
          wabs.nH  3.59648  10^22/cm^2  
            rs.kT  1.90914  keV  
            rs.norm  0.000150828  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            3.59648  -1.22896        +2.064        
            rs.kT            1.90914  -0.662458       +1.32776      
            rs.norm      0.000150828  -6.94575e-05    +9.93409e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            3.59648  -2.45927        +39.4529      
            rs.kT            1.90914  -1.78702        +14.7961      
            rs.norm      0.000150828  -0.000115911    +0.00897917   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 6.25423e-06 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.67779275,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.43989951,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    8.51843266811252,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1531' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:31:08> *** SUCCESS for Obsid=619  Ccdid=ACIS-I0  Srcid=7

**********************************************************************
***  Obsid=619  Srcid=8                                            ***
**********************************************************************
<2007-May-31 15:31:08> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 417.68493151 215.97945205 SKY 4283.2980656 5009.9629575
Background Event statistics: CHIP 2 414.66666667 199.38095238 SKY 4274.0798224 5023.0346912

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=193:224]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=193:224]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=193:224] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (4283.2980656,5009.9629575)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4283.2980656 sourcepixely=5009.9629575 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src8/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	3 	      @:	248 
   mean:	0.26996197719 
  sigma:	0.54748890858 
    sum:	142 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
142
Running dmstat
     infile=obs619/src8/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	18 
   mean:	0.030418250951 
  sigma:	0.18246989431 
    sum:	16 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
16
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.43988E+02
 powll:     converged to minimum =     1.10850E+02 at iteration =      3
 powll:    final statistic value =     1.10850E+02
    bkg_mdl_c1.factor  0.000657633     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.09676E+03
 powll:     converged to minimum =     4.18927E+02 at iteration =     16
 powll:    final statistic value =     4.18927E+02
          wabs.nH  4.30689  10^22/cm^2  
            rs.kT  2.1408  keV  
            rs.norm  0.00283228  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            4.30689  -0.426211       +0.475173     
            rs.kT             2.1408  -0.235024       +0.278536     
            rs.norm       0.00283228  -0.000364403    +0.000398751  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            4.30689  -1.02212        +1.19877      
            rs.kT             2.1408  -0.606372       +1.32058      
            rs.norm       0.00283228  -0.00128102     +0.00257157   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.000115549 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.60028151,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.41309339,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    141.407649301229,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.43988E+02
 powll:     converged to minimum =     1.10850E+02 at iteration =      3
 powll:    final statistic value =     1.10850E+02
    bkg_mdl_c1.factor  0.000657633     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.09676E+03
 powll:     converged to minimum =     4.18927E+02 at iteration =     22
 powll:    final statistic value =     4.18927E+02
          wabs.nH  4.30555  10^22/cm^2  
            rs.kT  2.14238  keV  
            rs.norm  0.00282941  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            4.30555  -0.426323       +0.474953     
            rs.kT            2.14238  -0.23549        +0.278885     
            rs.norm       0.00282941  -0.000364035    +0.000398348  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            4.30555  -1.02067        +1.20006      
            rs.kT            2.14238  -0.60791        +1.31924      
            rs.norm       0.00282941  -0.00127838     +0.00257461   

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:31:49 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 1564.22
 LVMQT: final statistic value = 6.18929 at iteration 13
          wabs.nH  3.76811  10^22/cm^2  
            rs.kT  2.40484  keV  
            rs.norm  0.00217056  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            3.76811  -0.499535       +0.64153      
            rs.kT            2.40484  -0.337095       +0.366867     
            rs.norm       0.00217056  -0.000311798    +0.000311805  

Struct_Type[3]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
NULL
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.00011133 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.60028151,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.41309339,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    141.407649301229,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Fitting model c_rs2
Running sherpa --batch c_rs2.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.43988E+02
 powll:     converged to minimum =     1.10850E+02 at iteration =      3
 powll:    final statistic value =     1.10850E+02
    bkg_mdl_c1.factor  0.000657633     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.09729E+03
 powll:     converged to minimum =     4.17632E+02 at iteration =     57
 powll:    final statistic value =     4.17632E+02
          wabs.nH  5.02946  10^22/cm^2  
            rs.kT  2.46686  keV  
            rs.norm  0.00223392  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.710899  keV  
           rs2.norm  0.00468077  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            5.02946  -0.433189       +0.478645     
            rs.kT            2.46686  -0.32564        +0.395207     
            rs.norm       0.00223392  -0.000357547    +0.000393816  
           rs2.kT           0.710899  -0.157443       +0.158661     
           rs2.norm       0.00468077  -0.00216921     +0.00249174   

Struct_Type[5]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: lower projection bound not found for  rs.kT 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 
WARNING: lower projection bound not found for  rs2.kT 
WARNING: upper projection bound not found for  rs2.kT 
Projection complete for parameter: rs2.kT 
WARNING: no change in statistic value (e.g. because of model truncation).
         Bound not determined for  rs2.norm 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            5.02946  -1.44622        +3.64154      
            rs.kT            2.46686  -2.45886        +61.5331      
            rs.norm       0.00223392  -0.0184874      +2101.54      
           rs2.kT           0.710899  -0.702899       +63.2891      
           rs2.norm       0.00468077  -28.9863          -----       

Struct_Type[5]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:32:06 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src8/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 3806.25
 LVMQT: final statistic value = 6.18929 at iteration 7
          wabs.nH  3.76805  10^22/cm^2  
            rs.kT  2.40503  keV  
            rs.norm  0.0021704  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.0239153  keV  
           rs2.norm  0.00601906  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();
WARNING: hit parameter space hard minimum for  rs2.kT 

WARNING: found better fit -- reminimizing!
 LVMQT: V2.0
 LVMQT: initial statistic value = 6.10483
 LVMQT: final statistic value = 5.12273 at iteration 13
          wabs.nH  5.20827  10^22/cm^2  
            rs.kT  2.21946  keV  
            rs.norm  0.00263695  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.402974  keV  
           rs2.norm  0.0198493  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs2.norm is equal to the rs2.norm.max limit boundary.
   You may wish to consider changing min/max values and refitting.


Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            5.20827  -0.504054       +0.622378     
            rs.kT            2.21946  -0.297929       +0.326074     
            rs.norm       0.00263695  -0.000427766    +0.000437071  
           rs2.kT           0.402974  -0.0937469      +0.0696068    
           rs2.norm        0.0198493  -0.0126785      +0.0140292    

Struct_Type[5]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
NULL
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs2"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs2.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs2.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.000110798 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.60028151,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.41309339,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    141.407649301229,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs2
Successfully updated c_rs2.mdl file
Successfully updated c_rs2.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1534' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><c_rs2.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:34:20> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=8

**********************************************************************
***  Obsid=619  Srcid=9                                            ***
**********************************************************************
<2007-May-31 15:34:20> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 511.78723404 13 SKY 4330.3105157 5240.545753
Background Event statistics: CHIP 2 526.875 71.075 SKY 4356.8946045 5172.9994751

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=1:32]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=513:768,chipy=65:96]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=257:512,chipy=1:32] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=513:768,chipy=65:96] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (4330.3105157,5240.545753)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4330.3105157 sourcepixely=5240.545753 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (4356.8946045,5172.9994751)
mkarf detsubsys=ACIS-I2 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=4356.8946045 sourcepixely=5172.9994751 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src9/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	119 
   mean:	0.085551330798 
  sigma:	0.29297928824 
    sum:	45 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
45
Running dmstat
     infile=obs619/src9/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	143 
   mean:	0.028517110266 
  sigma:	0.17749976354 
    sum:	15 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
15
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.66412E+02
 powll:     converged to minimum =     1.12711E+02 at iteration =      3
 powll:    final statistic value =     1.12711E+02
    bkg_mdl_c1.factor  0.00152478     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     4.63377E+02
 powll:     converged to minimum =     2.85187E+02 at iteration =     16
 powll:    final statistic value =     2.85187E+02
          wabs.nH  2.53126  10^22/cm^2  
            rs.kT  2.31541  keV  
            rs.norm  0.00123286  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.53126  -0.470887       +0.572969     
            rs.kT            2.31541  -0.509197       +0.731683     
            rs.norm       0.00123286  -0.000273056    +0.000320362  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.53126  -0.979604       +1.32664      
            rs.kT            2.31541  -0.910069       +3.20745      
            rs.norm       0.00123286  -0.000667888    +0.00174001   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 8.08773e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.59312396,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.38116051,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    44.4444099300095,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.66412E+02
 powll:     converged to minimum =     1.12711E+02 at iteration =      3
 powll:    final statistic value =     1.12711E+02
    bkg_mdl_c1.factor  0.00152478     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     4.63377E+02
 powll:     converged to minimum =     2.85187E+02 at iteration =     15
 powll:    final statistic value =     2.85187E+02
          wabs.nH  2.53286  10^22/cm^2  
            rs.kT  2.31541  keV  
            rs.norm  0.00123353  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.53286  -0.472122       +0.572754     
            rs.kT            2.31541  -0.509307       +0.730648     
            rs.norm       0.00123353  -0.000273204    +0.000320536  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.53286  -0.981126       +1.32498      
            rs.kT            2.31541  -0.910062       +3.20777      
            rs.norm       0.00123353  -0.000668531    +0.00173946   

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:35:20 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src9/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 47.5644
 LVMQT: final statistic value = 2.77272 at iteration 7
          wabs.nH  0.728724  10^22/cm^2  
            rs.kT  12.2018  keV  
            rs.norm  0.000462111  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();
WARNING: hit parameter space hard minimum for  wabs.nH 
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.728724    -----         +1.34832      
            rs.kT            12.2018  -9.13054          -----       
            rs.norm      0.000462111  -0.000138181    +0.000138182  

Struct_Type[3]
  if (1) run_unc()
WARNING: hit parameter space hard minimum for  wabs.nH 
Projection complete for parameter: wabs.nH 
NULL
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.000112619 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.59312396,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.38116051,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    44.4444099300095,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1535' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:35:35> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=9

**********************************************************************
***  Obsid=619  Srcid=10                                           ***
**********************************************************************
<2007-May-31 15:35:35> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 796.26415094 655.77358491 SKY 4738.6264372 4656.9040113
Background Event statistics: CHIP 2 775.125 664.775 SKY 4723.4580933 4644.269104

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=641:672]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=641:672]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=641:672] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (4738.6264372,4656.9040113)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4738.6264372 sourcepixely=4656.9040113 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src10/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	77 
   mean:	0.10076045627 
  sigma:	0.32529511555 
    sum:	53 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
53
Running dmstat
     infile=obs619/src10/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	14 
   mean:	0.022813688213 
  sigma:	0.14930915526 
    sum:	12 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
12
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.12889E+02
 powll:     converged to minimum =     9.02629E+01 at iteration =      3
 powll:    final statistic value =     9.02629E+01
    bkg_mdl_c1.factor  0.000588801     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     5.07822E+02
 powll:     converged to minimum =     3.04307E+02 at iteration =     11
 powll:    final statistic value =     3.04307E+02
          wabs.nH  1.60675  10^22/cm^2  
            rs.kT  7.85754  keV  
            rs.norm  0.000251227  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard minimum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.60675  -0.396579       +0.498097     
            rs.kT            7.85754    -----         +48.428       
            rs.norm      0.000251227  -5.16271e-05    +5.98218e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.60675  -0.791799       +1.04397      
            rs.kT            7.85754    -----         +56.1425      
            rs.norm      0.000251227  -7.94947e-05    +0.000247413  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 4.31788e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.53191597,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.46132909,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    52.4393256650803,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.12889E+02
 powll:     converged to minimum =     9.02629E+01 at iteration =      3
 powll:    final statistic value =     9.02629E+01
    bkg_mdl_c1.factor  0.000588801     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     5.07822E+02
 powll:     converged to minimum =     3.04307E+02 at iteration =     11
 powll:    final statistic value =     3.04307E+02
          wabs.nH  1.60655  10^22/cm^2  
            rs.kT  7.85936  keV  
            rs.norm  0.000251203  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard minimum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.60655  -0.396397       +0.49806      
            rs.kT            7.85936    -----         +48.4133      
            rs.norm      0.000251203  -5.16223e-05    +5.98161e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.60655  -0.791584       +1.0442       
            rs.kT            7.85936    -----         +56.1406      
            rs.norm      0.000251203  -7.94687e-05    +0.000247435  

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:36:12 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src10/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 41.6533
 LVMQT: final statistic value = 4.37129 at iteration 5
          wabs.nH  1.38017  10^22/cm^2  
            rs.kT  22.6246  keV  
            rs.norm  0.000206742  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 

WARNING: found better fit -- reminimizing!
 LVMQT: V2.0
 LVMQT: initial statistic value = 4.35756
 LVMQT: final statistic value = 4.34929 at iteration 2
          wabs.nH  1.34748  10^22/cm^2  
            rs.kT  25.7433  keV  
            rs.norm  0.000208034  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.34748  -0.715574       +1.16013      
            rs.kT            25.7433    -----           -----       
            rs.norm      0.000208034  -5.5269e-05     +5.52688e-05  

Struct_Type[3]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.34748  -0.719617       +1.75514      
            rs.kT            25.7433    -----           -----       
            rs.norm      0.000208034  -8.11459e-05    +0.000128615  

Struct_Type[3]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 4.08613e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.53191597,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.46132909,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    52.4393256650803,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1536' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:36:24> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=10

**********************************************************************
***  Obsid=619  Srcid=11                                           ***
**********************************************************************
<2007-May-31 15:36:24> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 815.75 628.46428571 SKY 4755.3818621 4691.0335868
Background Event statistics: CHIP 2 820.96551724 611.44827586 SKY 4754.1040881 4702.746279

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=609:640]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=609:640]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=609:640] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (4755.3818621,4691.0335868)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4755.3818621 sourcepixely=4691.0335868 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src11/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	129 
   mean:	0.10076045627 
  sigma:	0.32529511555 
    sum:	53 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
53
Running dmstat
     infile=obs619/src11/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	12 
   mean:	0.036121673004 
  sigma:	0.18659286627 
    sum:	19 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
19
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.77302E+02
 powll:     converged to minimum =     1.23865E+02 at iteration =      3
 powll:    final statistic value =     1.23865E+02
    bkg_mdl_c1.factor  0.00100406     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     7.04993E+02
 powll:     converged to minimum =     3.53243E+02 at iteration =      3
 powll:    final statistic value =     3.53243E+02
          wabs.nH  2.18263  10^22/cm^2  
            rs.kT  10  keV  
            rs.norm  0.000305906  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs.kT is equal to the rs.kT.max limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.18263  -0.520099       +0.660234     
            rs.kT                 10  -5.08219          -----       
            rs.norm      0.000305906  -6.36754e-05    +7.38145e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard maximum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.18263  -1.00826        +1.31819      
            rs.kT                 10  -13.806           -----       
            rs.norm      0.000305906  -8.85654e-05    +0.000310168  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 4.92879e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.52933944,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.45663017,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    52.1119905405015,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.77302E+02
 powll:     converged to minimum =     1.23865E+02 at iteration =      3
 powll:    final statistic value =     1.23865E+02
    bkg_mdl_c1.factor  0.00100406     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     7.04993E+02
 powll:     converged to minimum =     3.53131E+02 at iteration =      6
 powll:    final statistic value =     3.53131E+02
          wabs.nH  1.83625  10^22/cm^2  
            rs.kT  50  keV  
            rs.norm  0.00031998  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs.kT is equal to the rs.kT.max limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.83625  -0.488856       +0.622681     
            rs.kT                 50    -----           -----       
            rs.norm       0.00031998  -6.64745e-05    +7.70468e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.83625  -0.649068       +1.62176      
            rs.kT                 50    -----           -----       
            rs.norm       0.00031998  -0.000101627    +0.000125854  

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:36:59 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src11/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 5.42036
 LVMQT: final statistic value = 0.960081 at iteration 4
          wabs.nH  0.295992  10^22/cm^2  
            rs.kT  50  keV  
            rs.norm  0.000247343  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs.kT within 0.01% of the rs.kT.max limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type
  run_fit();
WARNING: hit parameter space hard minimum for  wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.295992    -----         +1.46521      
            rs.kT                 50    -----           -----       
            rs.norm      0.000247343  -6.39588e-05    +6.39588e-05  

Struct_Type[3]
  if (1) run_unc()
WARNING: hit parameter space hard minimum for  wabs.nH 
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.295992    -----         +2.13718      
            rs.kT                 50    -----           -----       
            rs.norm      0.000247343  -9.48187e-05    +0.000116867  

Struct_Type[3]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 6.8176e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.52933944,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.45663017,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    52.1119905405015,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1537' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:37:08> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=11

**********************************************************************
***  Obsid=619  Srcid=12                                           ***
**********************************************************************
<2007-May-31 15:37:08> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 1009.1971983 193.65301724 SKY 4862.9950993 5155.8258493
Background Event statistics: CHIP 2 936.2625 167.9875 SKY 4777.1130554 5162.1983093

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=193:224]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=161:192]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=193:224] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=161:192] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (4862.9950993,5155.8258493)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4862.9950993 sourcepixely=5155.8258493 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (4777.1130554,5162.1983093)
mkarf detsubsys=ACIS-I2 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=4777.1130554 sourcepixely=5162.1983093 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src12/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	14 	      @:	70 
   mean:	1.7547528517 
  sigma:	2.6868795129 
    sum:	923 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
923
Running dmstat
     infile=obs619/src12/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	4 
   mean:	0.098859315589 
  sigma:	0.31700630186 
    sum:	52 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
52
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     5.37375E+02
 powll:     converged to minimum =     2.48639E+02 at iteration =      3
 powll:    final statistic value =     2.48639E+02
    bkg_mdl_c1.factor  0.00426428     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     3.19388E+03
 powll:     converged to minimum =     6.67626E+02 at iteration =     14
 powll:    final statistic value =     6.67626E+02
          wabs.nH  0.894493  10^22/cm^2  
            rs.kT  2.71058  keV  
            rs.norm  0.00860865  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.894493  -0.0561717      +0.0585014    
            rs.kT            2.71058  -0.21778        +0.233989     
            rs.norm       0.00860865  -0.000445913    +0.000461912  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.894493  -0.118882       +0.126513     
            rs.kT            2.71058  -0.399278       +0.523809     
            rs.norm       0.00860865  -0.00116821     +0.00138739   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.00120025 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.51309478,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.39310752,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    921.075190596146,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     5.37375E+02
 powll:     converged to minimum =     2.48639E+02 at iteration =      3
 powll:    final statistic value =     2.48639E+02
    bkg_mdl_c1.factor  0.00426428     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     3.19388E+03
 powll:     converged to minimum =     6.67626E+02 at iteration =     14
 powll:    final statistic value =     6.67626E+02
          wabs.nH  0.894493  10^22/cm^2  
            rs.kT  2.71058  keV  
            rs.norm  0.00860865  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.894493  -0.0561717      +0.0585014    
            rs.kT            2.71058  -0.21778        +0.233989     
            rs.norm       0.00860865  -0.000445913    +0.000461912  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.894493  -0.118882       +0.126513     
            rs.kT            2.71058  -0.399278       +0.523809     
            rs.norm       0.00860865  -0.00116821     +0.00138739   

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:38:04 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 4003.32
 LVMQT: final statistic value = 96.8223 at iteration 6
          wabs.nH  0.821233  10^22/cm^2  
            rs.kT  3.0062  keV  
            rs.norm  0.00706958  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.821233  -0.0574628      +0.0643202    
            rs.kT             3.0062  -0.297876       +0.332433     
            rs.norm       0.00706958  -0.00039586     +0.000395861  

Struct_Type[3]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.821233  -0.118726       +0.155589     
            rs.kT             3.0062  -0.567438       +0.674288     
            rs.norm       0.00706958  -0.00100245     +0.00140741   

Struct_Type[3]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.00109224 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.51309478,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.39310752,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    921.075190596146,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Fitting model c_rs2
Running sherpa --batch c_rs2.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     5.37375E+02
 powll:     converged to minimum =     2.48639E+02 at iteration =      3
 powll:    final statistic value =     2.48639E+02
    bkg_mdl_c1.factor  0.00426428     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.56144E+03
 powll:     converged to minimum =     6.63203E+02 at iteration =     31
 powll:    final statistic value =     6.63203E+02
          wabs.nH  1.25635  10^22/cm^2  
            rs.kT  2.75733  keV  
            rs.norm  0.00814049  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.821925  keV  
           rs2.norm  0.00531773  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.25635  -0.0566466      +0.0590478    
            rs.kT            2.75733  -0.237768       +0.268341     
            rs.norm       0.00814049  -0.000537809    +0.00055838   
           rs2.kT           0.821925  -0.117401       +0.122681     
           rs2.norm       0.00531773  -0.000974721    +0.00102747   

Struct_Type[5]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.25635  -0.344512       +0.370951     
            rs.kT            2.75733  -0.496888       +0.747683     
            rs.norm       0.00814049  -0.00189576     +0.00207311   
           rs2.kT           0.821925  -0.162226       +0.270925     
           rs2.norm       0.00531773  -0.00470329     +0.0105558    

Struct_Type[5]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:38:17 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 38346.3
 LVMQT: final statistic value = 89.9815 at iteration 9
          wabs.nH  1.50589  10^22/cm^2  
            rs.kT  3.61263  keV  
            rs.norm  0.00571355  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.733129  keV  
           rs2.norm  0.0121651  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.50589  -0.0560619      +0.0629294    
            rs.kT            3.61263  -0.44089        +0.565102     
            rs.norm       0.00571355  -0.000497904    +0.000497908  
           rs2.kT           0.733129  -0.0530068      +0.0630241    
           rs2.norm        0.0121651  -0.0014534      +0.00145347   

Struct_Type[5]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.50589  -0.400322       +0.206992     
            rs.kT            3.61263  -1.05001        +3.68482      
            rs.norm       0.00571355  -0.00212743     +0.00226675   
           rs2.kT           0.733129  -0.0905363      +0.195532     
           rs2.norm        0.0121651  -0.00887461     +0.0078829    

Struct_Type[5]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs2"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs2.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs2.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.00110946 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.51309478,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.39310752,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    921.075190596146,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs2
Successfully updated c_rs2.mdl file
Successfully updated c_rs2.mdl file
Fitting model c_rs2a
Running sherpa --batch c_rs2a.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     5.37375E+02
 powll:     converged to minimum =     2.48639E+02 at iteration =      3
 powll:    final statistic value =     2.48639E+02
    bkg_mdl_c1.factor  0.00426428     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  rs.Abundanc.type=thaw
  rs2.Abundanc.type=thaw
  rs2.Abundanc => rs.Abundanc
  rs.kT.max=50
  source = (wabs * (rs+rs2))
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.56144E+03
 powll:     converged to minimum =     6.65793E+02 at iteration =     31
 powll:    final statistic value =     6.65793E+02
          wabs.nH  1.01423  10^22/cm^2  
            rs.kT  0.1361  keV  
            rs.Abundanc  0.291105     
            rs.norm  0.0628991  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  2.49313  keV  
           rs2.norm  0.00953843  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.01423  -0.0542183      +0.0568234    
            rs.kT             0.1361  -0.0311402      +0.00782184   
            rs.Abundanc     0.291105  -0.0803089      +0.0845495    
            rs.norm        0.0628991  -0.0497417      +0.0630237    
           rs2.kT            2.49313  -0.19447        +0.209958     
           rs2.norm       0.00953843  -0.000501122    +0.000519171  

Struct_Type[6]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: lower projection bound not found for  rs.kT 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.Abundanc 
Projection complete for parameter: rs.norm 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.01423  -0.193369       +0.328079     
            rs.kT             0.1361  -0.1281         +63.8639      
            rs.Abundanc     0.291105  -0.184464       +0.256305     
            rs.norm        0.0628991  -1.88029e+16    +9.17809e+18  
           rs2.kT            2.49313  -0.888686       +0.542325     
           rs2.norm       0.00953843  -0.00179994     +0.0172761    

Struct_Type[6]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:39:30 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src12/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  rs.Abundanc.type=thaw
  rs2.Abundanc.type=thaw
  rs2.Abundanc => rs.Abundanc
  rs.kT.max=50
  source = (wabs * (rs+rs2))
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 9821.84
 LVMQT: final statistic value = 94.953 at iteration 34
          wabs.nH  0.893768  10^22/cm^2  
            rs.kT  4.31558  keV  
            rs.Abundanc  0.401794     
            rs.norm  0.00424137  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  1.54011  keV  
           rs2.norm  0.00303627  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.893768  -0.0584014      +0.0650821    
            rs.kT            4.31558  -0.706527       +0.897081     
            rs.Abundanc     0.401794  -0.105233       +0.105288     
            rs.norm       0.00424137  -0.000353344    +0.000353633  
           rs2.kT            1.54011  -0.307339       +0.376585     
           rs2.norm       0.00303627  -0.000475665    +0.000475695  

Struct_Type[6]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
WARNING: lower projection bound not found for  rs.kT 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.Abundanc 
Projection complete for parameter: rs.norm 
WARNING: lower projection bound not found for  rs2.kT 
WARNING: upper projection bound not found for  rs2.kT 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.893768  -0.163646       +0.89229      
            rs.kT            4.31558  -4.30758        +59.6844      
            rs.Abundanc     0.401794  -0.772409       +2.12746      
            rs.norm       0.00424137  -0.0165952      +0.00436404   
           rs2.kT            1.54011  -1.53211        +62.4599      
           rs2.norm       0.00303627  -0.00822496     +0.00489421   

Struct_Type[6]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs2a"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs2a.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs2a.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.0011107 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.51309478,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.39310752,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    921.075190596146,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs2a
Successfully updated c_rs2a.mdl file
Successfully updated c_rs2a.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1543' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><c_rs2.ps><c_rs2a.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:43:56> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=12

**********************************************************************
***  Obsid=619  Srcid=13                                           ***
**********************************************************************
<2007-May-31 15:43:56> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 905.28205128 935.98290598 SKY 4905.7494616 4405.7472372
Background Event statistics: CHIP 2 885.11627907 945.48837209 SKY 4905.6456895 4395.1061274

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=929:960]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=929:960]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=769:1024,chipy=929:960] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (4905.7494616,4405.7472372)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4905.7494616 sourcepixely=4405.7472372 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src13/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	4 	      @:	92 
   mean:	0.22243346008 
  sigma:	0.55663178601 
    sum:	117 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
117
Running dmstat
     infile=obs619/src13/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	10 
   mean:	0.032319391635 
  sigma:	0.17684696367 
    sum:	17 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
17
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.59450E+02
 powll:     converged to minimum =     1.19890E+02 at iteration =      3
 powll:    final statistic value =     1.19890E+02
    bkg_mdl_c1.factor  0.000708296     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     6.07330E+02
 powll:     converged to minimum =     3.67546E+02 at iteration =     12
 powll:    final statistic value =     3.67546E+02
          wabs.nH  1.08935  10^22/cm^2  
            rs.kT  2.17244  keV  
            rs.norm  0.000691196  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.08935  -0.159217       +0.176781     
            rs.kT            2.17244  -0.381754       +0.525021     
            rs.norm      0.000691196  -9.75792e-05    +0.00010776   

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.08935  -0.337507       +0.399713     
            rs.kT            2.17244  -0.613816       +1.24286      
            rs.norm      0.000691196  -0.000230878    +0.000383444  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 7.54839e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.50673663,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.49562247,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    116.370334940603,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.59450E+02
 powll:     converged to minimum =     1.19890E+02 at iteration =      3
 powll:    final statistic value =     1.19890E+02
    bkg_mdl_c1.factor  0.000708296     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     6.07330E+02
 powll:     converged to minimum =     3.67546E+02 at iteration =     12
 powll:    final statistic value =     3.67546E+02
          wabs.nH  1.08928  10^22/cm^2  
            rs.kT  2.17253  keV  
            rs.norm  0.000691153  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.08928  -0.159199       +0.176796     
            rs.kT            2.17253  -0.381759       +0.525078     
            rs.norm      0.000691153  -9.75731e-05    +0.000107753  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.08928  -0.337443       +0.399781     
            rs.kT            2.17253  -0.613938       +1.24275      
            rs.norm      0.000691153  -0.000230833    +0.000383483  

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:44:33 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 166.156
 LVMQT: final statistic value = 6.42832 at iteration 5
          wabs.nH  0.947002  10^22/cm^2  
            rs.kT  2.1273  keV  
            rs.norm  0.000612006  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.947002  -0.200239       +0.25681      
            rs.kT             2.1273  -0.444281       +0.544468     
            rs.norm      0.000612006  -9.7586e-05     +9.76028e-05  

Struct_Type[3]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.947002  -1.46997        +0.709807     
            rs.kT             2.1273  -0.832414       +2.63232      
            rs.norm      0.000612006  -0.000303807    +0.000619713  

Struct_Type[3]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 7.21187e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.50673663,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.49562247,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    116.370334940603,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Fitting model c_rs2
Running sherpa --batch c_rs2.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.59450E+02
 powll:     converged to minimum =     1.19890E+02 at iteration =      3
 powll:    final statistic value =     1.19890E+02
    bkg_mdl_c1.factor  0.000708296     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     6.06980E+02
 powll:     converged to minimum =     3.67329E+02 at iteration =     24
 powll:    final statistic value =     3.67329E+02
          wabs.nH  1.2058  10^22/cm^2  
            rs.kT  1.26512  keV  
            rs.norm  0.000400896  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  2.83988  keV  
           rs2.norm  0.000396215  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             1.2058  -0.159975       +0.177485     
            rs.kT            1.26512  -0.357636       +0.612186     
            rs.norm      0.000400896  -0.000136101    +0.000152918  
           rs2.kT            2.83988  -0.745487       +1.1771       
           rs2.norm      0.000396215  -9.03872e-05    +0.000100373  

Struct_Type[5]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: lower projection bound not found for  rs.kT 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
WARNING: no change in statistic value (e.g. because of model truncation).
         Bound not determined for  rs.norm 
WARNING: no change in statistic value (e.g. because of model truncation).
         Bound not determined for  rs.norm 
Projection complete for parameter: rs.norm 
WARNING: lower projection bound not found for  rs2.kT 
WARNING: upper projection bound not found for  rs2.kT 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             1.2058  -3.18228        +2.13827      
            rs.kT            1.26512  -1.25712        +62.7349      
            rs.norm      0.000400896    -----           -----       
           rs2.kT            2.83988  -2.83188        +61.1601      
           rs2.norm      0.000396215  -0.00181704     +0.000735559  

Struct_Type[5]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:44:45 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src13/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 232.977
 LVMQT: final statistic value = 5.96658 at iteration 9
          wabs.nH  1.06236  10^22/cm^2  
            rs.kT  1.46024  keV  
            rs.norm  0.00061816  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  10.7953  keV  
           rs2.norm  0.000103016  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard minimum for  rs2.kT 
WARNING: hit parameter space hard maximum for  rs2.kT 

WARNING: found better fit -- reminimizing!
 LVMQT: V2.0
 LVMQT: initial statistic value = 5.9565
 LVMQT: final statistic value = 5.93686 at iteration 6
          wabs.nH  1.07666  10^22/cm^2  
            rs.kT  1.44357  keV  
            rs.norm  0.000640359  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  15.0456  keV  
           rs2.norm  9.96067e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING: hit parameter space hard minimum for  rs2.kT 
WARNING: hit parameter space hard maximum for  rs2.kT 

WARNING: found better fit -- reminimizing!
 LVMQT: V2.0
 LVMQT: initial statistic value = 5.92683
 LVMQT: final statistic value = 5.92098 at iteration 4
          wabs.nH  1.07818  10^22/cm^2  
            rs.kT  1.44316  keV  
            rs.norm  0.000648734  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  20.9697  keV  
           rs2.norm  9.84468e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING: hit parameter space hard minimum for  rs2.kT 
WARNING: hit parameter space hard maximum for  rs2.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.07818  -0.200811       +0.257413     
            rs.kT            1.44316  -0.315867       +0.332571     
            rs.norm      0.000648734  -0.000131469    +0.000131647  
           rs2.kT            20.9697    -----           -----       
           rs2.norm      9.84468e-05  -5.83537e-05    +5.77146e-05  

Struct_Type[5]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 
WARNING: hit parameter space hard minimum for  rs2.kT 
WARNING: hit parameter space hard maximum for  rs2.kT 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.07818  -1.47257        +0.891973     
            rs.kT            1.44316  -0.768024       +62.5568      
            rs.norm      0.000648734  -0.000404403    +0.00158387   
           rs2.kT            20.9697    -----           -----       
           rs2.norm      9.84468e-05  -0.00257345     +0.000172471  

Struct_Type[5]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs2"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs2.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs2.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 7.50267e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.50673663,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.49562247,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    116.370334940603,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs2
Successfully updated c_rs2.mdl file
Successfully updated c_rs2.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1546' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><c_rs2.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:46:12> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=13

**********************************************************************
***  Obsid=619  Srcid=14                                           ***
**********************************************************************
<2007-May-31 15:46:12> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 3 30.452631579 1008.6631579 SKY 5018.2168586 4308.1964227
Background Event statistics: CHIP 3 495.44827586 979.20689655 SKY 5006.3113046 4312.5120723

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=1:256,chipy=993:1024]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=257:512,chipy=961:992]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=1:256,chipy=993:1024] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=257:512,chipy=961:992] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=3]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (5018.2168586,4308.1964227)
mkarf detsubsys=ACIS-I3 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=5018.2168586 sourcepixely=4308.1964227 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (5006.3113046,4312.5120723)
mkarf detsubsys=ACIS-I3 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=5006.3113046 sourcepixely=4312.5120723 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src14/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	3 	      @:	72 
   mean:	0.18060836502 
  sigma:	0.47332294565 
    sum:	95 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
95
Running dmstat
     infile=obs619/src14/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	13 
   mean:	0.026615969582 
  sigma:	0.16095825467 
    sum:	14 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
14
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.30939E+02
 powll:     converged to minimum =     9.75288E+01 at iteration =      3
 powll:    final statistic value =     9.75288E+01
    bkg_mdl_c1.factor  0.000789796     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     4.94977E+02
 powll:     converged to minimum =     3.40749E+02 at iteration =      5
 powll:    final statistic value =     3.40749E+02
          wabs.nH  0.498941  10^22/cm^2  
            rs.kT  3.71327  keV  
            rs.norm  0.000425799  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.498941  -0.127011       +0.145942     
            rs.kT            3.71327  -1.01363        +2.0393       
            rs.norm      0.000425799  -6.6326e-05     +7.40471e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.498941  -0.222324       +0.279298     
            rs.kT            3.71327  -1.42315        +4.85386      
            rs.norm      0.000425799  -0.00012285     +0.000201468  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 9.22848e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.48987740,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.50891895,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    94.4815143360362,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.30939E+02
 powll:     converged to minimum =     9.75288E+01 at iteration =      3
 powll:    final statistic value =     9.75288E+01
    bkg_mdl_c1.factor  0.000789796     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     4.94977E+02
 powll:     converged to minimum =     3.40749E+02 at iteration =      5
 powll:    final statistic value =     3.40749E+02
          wabs.nH  0.498941  10^22/cm^2  
            rs.kT  3.71327  keV  
            rs.norm  0.000425799  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.498941  -0.127011       +0.145942     
            rs.kT            3.71327  -1.01363        +2.0393       
            rs.norm      0.000425799  -6.6326e-05     +7.40471e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.498941  -0.222324       +0.279298     
            rs.kT            3.71327  -1.42315        +4.85386      
            rs.norm      0.000425799  -0.00012285     +0.000201468  

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:47:06 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src14/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 22.1595
 LVMQT: final statistic value = 2.48892 at iteration 5
          wabs.nH  0.612943  10^22/cm^2  
            rs.kT  3.33913  keV  
            rs.norm  0.000461269  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.612943  -0.194427       +0.259629     
            rs.kT            3.33913  -1.09169        +1.82943      
            rs.norm      0.000461269  -8.25608e-05    +8.25615e-05  

Struct_Type[3]
  if (1) run_unc()
WARNING: lower projection bound not found for  wabs.nH 
Projection complete for parameter: wabs.nH 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.612943  -0.612943       +0.806005     
            rs.kT            3.33913  -1.81041        +60.6609      
            rs.norm      0.000461269  -0.000221497    +0.000560893  

Struct_Type[3]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 8.66314e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.48987740,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.50891895,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    94.4815143360362,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1547' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:47:17> *** SUCCESS for Obsid=619  Ccdid=ACIS-I3  Srcid=14

**********************************************************************
***  Obsid=619  Srcid=15                                           ***
**********************************************************************
<2007-May-31 15:47:17> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 0 23.608695652 141.82608696 SKY 2861.2090056 4783.4976223
Background Event statistics: CHIP 0 102.97916667 170.3125 SKY 2942.9216054 4776.6088511

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=1:256,chipy=129:160]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=1:256,chipy=161:192]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=1:256,chipy=129:160] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=1:256,chipy=161:192] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=0]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (2861.2090056,4783.4976223)
mkarf detsubsys=ACIS-I0 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=2861.2090056 sourcepixely=4783.4976223 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (2942.9216054,4776.6088511)
mkarf detsubsys=ACIS-I0 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=2942.9216054 sourcepixely=4776.6088511 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src15/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	19 
   mean:	0.034220532319 
  sigma:	0.18179518004 
    sum:	18 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
18
Running dmstat
     infile=obs619/src15/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	3 
   mean:	0.057034220532 
  sigma:	0.23190799516 
    sum:	30 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
30
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src15/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     2.79667E+02
 powll:     converged to minimum =     1.77842E+02 at iteration =      3
 powll:    final statistic value =     1.77842E+02
    bkg_mdl_c1.factor  0.00137992     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     3.35270E+02
 powll:     converged to minimum =     2.77816E+02 at iteration =     28
 powll:    final statistic value =     2.77816E+02
          wabs.nH  4.31277  10^22/cm^2  
            rs.kT  0.773397  keV  
            rs.norm  0.00161377  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            4.31277  -0.753031       +0.957069     
            rs.kT           0.773397  -0.122711       +0.148682     
            rs.norm       0.00161377  -0.000577395    +0.000750773  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            4.31277  -5.55463        +2.60303      
            rs.kT           0.773397  -0.314338       +2.24111      
            rs.norm       0.00161377  -0.00149839     +0.0162246    

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 1.19364e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.81437676,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.44348565,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    16.8889693891259,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1548' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:48:23> *** SUCCESS for Obsid=619  Ccdid=ACIS-I0  Srcid=15

**********************************************************************
***  Obsid=619  Srcid=16                                           ***
**********************************************************************
<2007-May-31 15:48:23> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 1 773.09090909 839.36363636 SKY 3309.8917569 3771.0267001
Background Event statistics: CHIP 1 764.82142857 843.80357143 SKY 3313.2023315 3772.1967032

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=1,chipx=769:1024,chipy=833:864]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=1,chipx=513:768,chipy=833:864]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=1,chipx=769:1024,chipy=833:864] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=1,chipx=513:768,chipy=833:864] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=1]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (3309.8917569,3771.0267001)
mkarf detsubsys=ACIS-I1 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=3309.8917569 sourcepixely=3771.0267001 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (3313.2023315,3772.1967032)
mkarf detsubsys=ACIS-I1 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=3313.2023315 sourcepixely=3772.1967032 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src16/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	126 
   mean:	0.020912547529 
  sigma:	0.14309162409 
    sum:	11 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
11
Running dmstat
     infile=obs619/src16/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	50 
   mean:	0.030418250951 
  sigma:	0.17173520594 
    sum:	16 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
16
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src16/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.44237E+02
 powll:     converged to minimum =     1.12746E+02 at iteration =      3
 powll:    final statistic value =     1.12746E+02
    bkg_mdl_c1.factor  0.000618709     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.76332E+02
 powll:     converged to minimum =     1.90943E+02 at iteration =     15
 powll:    final statistic value =     1.90943E+02
          wabs.nH  4.43418  10^22/cm^2  
            rs.kT  4.29151  keV  
            rs.norm  0.000118774  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            4.43418  -1.66441        +2.57461      
            rs.kT            4.29151  -1.99404          -----       
            rs.norm      0.000118774  -5.04699e-05    +6.98629e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard maximum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            4.43418  -1.67544        +7.00428      
            rs.kT            4.29151  -2.00897          -----       
            rs.norm      0.000118774  -8.04152e-05    +0.00231803   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 9.3853e-06 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.74710361,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.58219137,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    10.4071460627849,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1549' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:49:23> *** SUCCESS for Obsid=619  Ccdid=ACIS-I1  Srcid=16

**********************************************************************
***  Obsid=619  Srcid=17                                           ***
**********************************************************************
<2007-May-31 15:49:23> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 0 593.5 226.15384615 SKY 3438.1634897 4822.7647423
Background Event statistics: CHIP 0 613.11926606 222.22018349 SKY 3452.8625242 4829.6794187

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=513:768,chipy=225:256]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=513:768,chipy=193:224]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=513:768,chipy=225:256] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=513:768,chipy=193:224] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=0]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (3438.1634897,4822.7647423)
mkarf detsubsys=ACIS-I0 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=3438.1634897 sourcepixely=4822.7647423 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (3452.8625242,4829.6794187)
mkarf detsubsys=ACIS-I0 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=3452.8625242 sourcepixely=4829.6794187 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src17/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	77 
   mean:	0.045627376426 
  sigma:	0.20867563094 
    sum:	24 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
24
Running dmstat
     infile=obs619/src17/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	4 
   mean:	0.057034220532 
  sigma:	0.23190799516 
    sum:	30 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
30
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src17/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     2.77381E+02
 powll:     converged to minimum =     1.72558E+02 at iteration =      3
 powll:    final statistic value =     1.72558E+02
    bkg_mdl_c1.factor  0.00145615     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     3.89600E+02
 powll:     converged to minimum =     2.87800E+02 at iteration =     17
 powll:    final statistic value =     2.87800E+02
          wabs.nH  2.70844  10^22/cm^2  
            rs.kT  1.40766  keV  
            rs.norm  0.000467414  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.70844  -0.567225       +0.70635      
            rs.kT            1.40766  -0.319619       +0.414848     
            rs.norm      0.000467414  -0.00014479     +0.000181232  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.70844  -1.26959        +1.95618      
            rs.kT            1.40766  -0.703625       +1.90874      
            rs.norm      0.000467414  -0.000315787    +0.00249197   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 1.69015e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.72683528,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.43882330,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    22.8007312688099,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1550' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:50:25> *** SUCCESS for Obsid=619  Ccdid=ACIS-I0  Srcid=17

**********************************************************************
***  Obsid=619  Srcid=18                                           ***
**********************************************************************
<2007-May-31 15:50:25> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 1 570.71428571 370 SKY 3594.0696847 3348.5656738
Background Event statistics: CHIP 1 584.92857143 355.71428571 SKY 3589.0061384 3338.4473819

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=1,chipx=513:768,chipy=353:384]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=1,chipx=513:768,chipy=353:384]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=1,chipx=513:768,chipy=353:384] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=1]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (3594.0696847,3348.5656738)
mkarf detsubsys=ACIS-I1 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=3594.0696847 sourcepixely=3348.5656738 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src18/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	63 
   mean:	0.011406844106 
  sigma:	0.1061919395 
    sum:	6 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
6
Running dmstat
     infile=obs619/src18/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	94 
   mean:	0.026615969582 
  sigma:	0.16095825467 
    sum:	14 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
14
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src18/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.25553E+02
 powll:     converged to minimum =     1.00140E+02 at iteration =      3
 powll:    final statistic value =     1.00140E+02
    bkg_mdl_c1.factor  0.000564281     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.64725E+02
 powll:     converged to minimum =     1.36164E+02 at iteration =     16
 powll:    final statistic value =     1.36164E+02
          wabs.nH  1.52742  10^22/cm^2  
            rs.kT  0.900269  keV  
            rs.norm  9.00536e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.52742  -0.501979       +0.739683     
            rs.kT           0.900269  -0.330354       +0.45192      
            rs.norm      9.00536e-05  -4.7875e-05     +7.41817e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.52742  -1.25101        +7.15532      
            rs.kT           0.900269  -0.332759       +2.22063      
            rs.norm      9.00536e-05  -7.47638e-05    +0.0111034    

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 3.58779e-06 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.70369813,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.64005510,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    5.48170963958378,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1551' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:51:12> *** SUCCESS for Obsid=619  Ccdid=ACIS-I1  Srcid=18

**********************************************************************
***  Obsid=619  Srcid=19                                           ***
**********************************************************************
<2007-May-31 15:51:12> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 3 296.5 269.16666667 SKY 4916.8457031 3529.5599772
Background Event statistics: CHIP 3 282.52873563 261.17241379 SKY 4926.6529948 3522.9790853

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=257:512,chipy=257:288]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=257:512,chipy=257:288]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=3,chipx=257:512,chipy=257:288] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=3]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (4916.8457031,3529.5599772)
mkarf detsubsys=ACIS-I3 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4916.8457031 sourcepixely=3529.5599772 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src19/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	100 
   mean:	0.0076045627376 
  sigma:	0.086871936569 
    sum:	4 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
4
Running dmstat
     infile=obs619/src19/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	35 
   mean:	0.06463878327 
  sigma:	0.26089303115 
    sum:	34 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
34
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src19/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     3.12647E+02
 powll:     converged to minimum =     1.97564E+02 at iteration =      3
 powll:    final statistic value =     1.97564E+02
    bkg_mdl_c1.factor  0.00137299     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     3.01284E+02
 powll:     converged to minimum =     2.34426E+02 at iteration =     13
 powll:    final statistic value =     2.34426E+02
          wabs.nH  2.06415  10^22/cm^2  
            rs.kT  10  keV  
            rs.norm  1.65509e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs.kT is equal to the rs.kT.max limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard minimum for  wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.06415    -----         +4.85815      
            rs.kT                 10    -----           -----       
            rs.norm      1.65509e-05  -1.28514e-05    +2.22051e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
WARNING: hit parameter space hard minimum for  wabs.nH 
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.06415    -----         +5.94702      
            rs.kT                 10    -----           -----       
            rs.norm      1.65509e-05  -1.39571e-05    +8.5576e-05   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 2.72517e-06 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.50470069,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.61442130,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    2.74058773789203,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1551' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:51:45> *** SUCCESS for Obsid=619  Ccdid=ACIS-I3  Srcid=19

**********************************************************************
***  Obsid=619  Srcid=20                                           ***
**********************************************************************
<2007-May-31 15:51:45> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 0 441.9375 238.1875 SKY 3286.704895 4779.0282288
Background Event statistics: CHIP 0 428.82758621 223.75862069 SKY 3273.1617474 4789.9071704

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=257:512,chipy=225:256]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=257:512,chipy=193:224]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=257:512,chipy=225:256] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=0,chipx=257:512,chipy=193:224] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=0]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (3286.704895,4779.0282288)
mkarf detsubsys=ACIS-I0 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=3286.704895 sourcepixely=4779.0282288 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (3273.1617474,4789.9071704)
mkarf detsubsys=ACIS-I0 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=3273.1617474 sourcepixely=4789.9071704 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src20/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	105 
   mean:	0.020912547529 
  sigma:	0.14309162409 
    sum:	11 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
11
Running dmstat
     infile=obs619/src20/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	4 
   mean:	0.043726235741 
  sigma:	0.20448533456 
    sum:	23 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
23
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src20/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     2.08319E+02
 powll:     converged to minimum =     1.43312E+02 at iteration =      3
 powll:    final statistic value =     1.43312E+02
    bkg_mdl_c1.factor  0.00101185     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     3.05193E+02
 powll:     converged to minimum =     2.21694E+02 at iteration =      6
 powll:    final statistic value =     2.21694E+02
          wabs.nH  4.8021  10^22/cm^2  
            rs.kT  10  keV  
            rs.norm  9.04688e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs.kT within 0.01% of the rs.kT.max limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             4.8021  -2.0405         +3.48986      
            rs.kT                 10    -----           -----       
            rs.norm      9.04688e-05  -3.98152e-05    +5.55755e-05  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
WARNING: hit parameter space hard minimum for  rs.kT 
WARNING: hit parameter space hard maximum for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             4.8021  -5.50137        +12.1343      
            rs.kT                 10    -----           -----       
            rs.norm      9.04688e-05  -4.98042e-05    +0.000873031  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 1.04777e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.75004595,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.44447192,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    10.0790329668282,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1552' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:52:42> *** SUCCESS for Obsid=619  Ccdid=ACIS-I0  Srcid=20

**********************************************************************
***  Obsid=619  Srcid=21                                           ***
**********************************************************************
<2007-May-31 15:52:42> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 2 179.08333333 16.833333333 SKY 4006.555776 5168.2767131
Background Event statistics: CHIP 2 200.35 77.4 SKY 4037.4508179 5105.4128662

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=1:256,chipy=1:32]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=1:256,chipy=65:96]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=1:256,chipy=1:32] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=2,chipx=1:256,chipy=65:96] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=2]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (4006.555776,5168.2767131)
mkarf detsubsys=ACIS-I2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=4006.555776 sourcepixely=5168.2767131 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (4037.4508179,5105.4128662)
mkarf detsubsys=ACIS-I2 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=4037.4508179 sourcepixely=5105.4128662 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf
Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src21/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	2 	      @:	96 
   mean:	0.043726235741 
  sigma:	0.22230342954 
    sum:	23 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
23
Running dmstat
     infile=obs619/src21/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	1 	      @:	10 
   mean:	0.01711026616 
  sigma:	0.1296823232 
    sum:	9 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
9
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src21/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     9.47485E+01
 powll:     converged to minimum =     7.34534E+01 at iteration =      3
 powll:    final statistic value =     7.34534E+01
    bkg_mdl_c1.factor  0.000780655     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.45143E+02
 powll:     converged to minimum =     1.67935E+02 at iteration =     15
 powll:    final statistic value =     1.67935E+02
          wabs.nH  2.41587  10^22/cm^2  
            rs.kT  1.14008  keV  
            rs.norm  0.00101663  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.41587  -0.458453       +0.561649     
            rs.kT            1.14008  -0.206281       +0.282967     
            rs.norm       0.00101663  -0.000304255    +0.000379994  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.41587  -1.01526        +1.38478      
            rs.kT            1.14008  -0.510603       +0.747944     
            rs.norm       0.00101663  -0.000636861    +0.0044566    

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 3.1594e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.64158676,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.39152265,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    22.6666768680942,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1553' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:53:40> *** SUCCESS for Obsid=619  Ccdid=ACIS-I2  Srcid=21

**********************************************************************
***  Obsid=619  Srcid=22                                           ***
**********************************************************************
<2007-May-31 15:53:40> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 6 405.62727273 665.44545455 SKY 5555.351851 5280.0329901
Background Event statistics: CHIP 6 404.31377551 670.55102041 SKY 5548.7215582 5278.9795271

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=6,chipx=257:512,chipy=641:672]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=6,chipx=257:512,chipy=641:672]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are the same
Building common RMFs and ARFs for source and background spectra

Make RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=6,chipx=257:512,chipy=641:672] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2

Created RMF file acis.rmf

Running asphist to create aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=6]" clobber=yes dtffile="" verbose=0
Running mkarf to create acis.arf at (5555.351851,5280.0329901)
mkarf detsubsys=ACIS-S2 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=5555.351851 sourcepixely=5280.0329901 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf

# psextract: WARNING: For ccd_id=6 and CTI_APP=PPPPPBPBPP keyword value,
you should be using the mkacisrmf tool. The source RMF
created with mkrmf is INCORRECT for your analysis.
Run mkacisrmf independently to create a new RMF:
http://cxc.harvard.edu/ciao/threads/mkacisrmf/


# psextract: WARNING: For ccd_id=6 and CTI_APP=PPPPPBPBPP keyword value,
you should be using the mkacisrmf tool. The background RMF
created with mkrmf is INCORRECT for your analysis.
Run mkacisrmf independently to create a new RMF:
http://cxc.harvard.edu/ciao/threads/mkacisrmf/

Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src22/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	3 	      @:	99 
   mean:	0.17870722433 
  sigma:	0.46798963483 
    sum:	94 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
94
Running dmstat
     infile=obs619/src22/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	5 	      @:	47 
   mean:	0.4752851711 
  sigma:	0.69103260369 
    sum:	250 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
250
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     2.42159E+03
 powll:     converged to minimum =     5.10349E+02 at iteration =      3
 powll:    final statistic value =     5.10349E+02
    bkg_mdl_c1.factor  0.012327     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.16573E+03
 powll:     converged to minimum =     7.82584E+02 at iteration =     12
 powll:    final statistic value =     7.82584E+02
          wabs.nH  2.78407  10^22/cm^2  
            rs.kT  2.31542  keV  
            rs.norm  0.00127046  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.78407  -0.365781       +0.422254     
            rs.kT            2.31542  -0.413558       +0.530762     
            rs.norm       0.00127046  -0.000212593    +0.000237849  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.78407  -0.804936       +1.07024      
            rs.kT            2.31542  -0.854834       +2.27476      
            rs.norm       0.00127046  -0.000582143    +0.00143778   

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 7.798e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.40990178,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.37607952,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    84.7405088759973,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-I.IN
#
# Empirically derived background model for the ACIS-I detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-I background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 7.65748e-05
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.97202e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 8.22613e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 8.22051e-06
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 8.37722e-06
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.81009e-07
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -7.19994e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 4.00101e-08
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.36288e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.172436
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.527575
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 0
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.000566705
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = -0.0001
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = -2.38881e-05
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.00032534
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.148224
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.46063
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000924119
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0001
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.0133502
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.71465
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.190619
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.5
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88978e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     2.42159E+03
 powll:     converged to minimum =     5.10349E+02 at iteration =      3
 powll:    final statistic value =     5.10349E+02
    bkg_mdl_c1.factor  0.012327     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.16573E+03
 powll:     converged to minimum =     7.82584E+02 at iteration =     22
 powll:    final statistic value =     7.82584E+02
          wabs.nH  2.78209  10^22/cm^2  
            rs.kT  2.31541  keV  
            rs.norm  0.00126963  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.78209  -0.364979       +0.423187     
            rs.kT            2.31541  -0.413174       +0.531849     
            rs.norm       0.00126963  -0.000212454    +0.000237694  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.78209  -0.802982       +1.07223      
            rs.kT            2.31541  -0.854606       +2.27448      
            rs.norm       0.00126963  -0.000581658    +0.00143859   

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:54:17 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src22/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 452.833
 LVMQT: final statistic value = 5.0845 at iteration 7
          wabs.nH  2.37168  10^22/cm^2  
            rs.kT  2.51901  keV  
            rs.norm  0.00100477  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            2.37168  -0.447571       +0.609136     
            rs.kT            2.51901  -0.580059       +0.679464     
            rs.norm       0.00100477  -0.00019249     +0.000192488  

Struct_Type[3]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
NULL
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 7.40597e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.40990178,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.37607952,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    84.7405088759973,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1554' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:54:33> *** SUCCESS for Obsid=619  Ccdid=ACIS-S2  Srcid=22

**********************************************************************
***  Obsid=619  Srcid=23                                           ***
**********************************************************************
<2007-May-31 15:54:33> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 7 291.64236111 463.01388889 SKY 5942.9268324 4411.4780714
Background Event statistics: CHIP 7 419.95437788 475.26981567 SKY 5950.5770249 4313.77651

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=289:320,chipy=449:480]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=417:448,chipy=449:480]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=289:320,chipy=449:480] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2
Contents of mkrmf log file:

	*** mkrmf parameter inputs ***
	          input file: /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=289:320,chipy=449:480]
	         output file: acis.rmf
	        weights file: 
	               axis1: energy=0.1:11.0:0.01
	               axis2: pi=1:1024:1
	            log file: ./.psp.mlog
	               axis3: none
	               axis4: none
	               axis5: none
	           threshold: 1.00e-05
	        output formt: legacy
	clobber(1=yes, 0=no): 1
	       verbose level: 2


ATTEN:  The final MATRIX grids along "ENERGY" axis will be bound in 
		0.220000--11.000000 rather than the user-defined range 
		0.100000--11.000000.

	The final grid range of the above is to fit to FEF grid bounds, 
	but the bin size specified by user will be reduced by 12.


Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=417:448,chipy=449:480] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2
mkrmf error log:

	*** mkrmf parameter inputs ***
	          input file: /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=417:448,chipy=449:480]
	         output file: acis_bg.rmf
	        weights file: 
	               axis1: energy=0.1:11.0:0.01
	               axis2: pi=1:1024:1
	            log file: ./.psp.bgmlog
	               axis3: none
	               axis4: none
	               axis5: none
	           threshold: 1.00e-05
	        output formt: legacy
	clobber(1=yes, 0=no): 1
	       verbose level: 2


ATTEN:  The final MATRIX grids along "ENERGY" axis will be bound in 
		0.220000--11.000000 rather than the user-defined range 
		0.100000--11.000000.

	The final grid range of the above is to fit to FEF grid bounds, 
	but the bin size specified by user will be reduced by 12.


Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=7]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (5942.9268324,4411.4780714)
mkarf detsubsys=ACIS-S3 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=5942.9268324 sourcepixely=4411.4780714 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (5950.5770249,4313.77651)
mkarf detsubsys=ACIS-S3 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=5950.5770249 sourcepixely=4313.77651 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf

# psextract: WARNING: For ccd_id=7 and CTI_APP=PPPPPBPBPP keyword value,
you should be using the mkacisrmf tool. The source RMF
created with mkrmf is INCORRECT for your analysis.
Run mkacisrmf independently to create a new RMF:
http://cxc.harvard.edu/ciao/threads/mkacisrmf/


# psextract: WARNING: For ccd_id=7 and CTI_APP=PPPPPBPBPP keyword value,
you should be using the mkacisrmf tool. The background RMF
created with mkrmf is INCORRECT for your analysis.
Run mkacisrmf independently to create a new RMF:
http://cxc.harvard.edu/ciao/threads/mkacisrmf/

Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src23/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	1 
    max:	5 	      @:	94 
   mean:	0.33650190114 
  sigma:	0.68863556546 
    sum:	177 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
177
Running dmstat
     infile=obs619/src23/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	135 
    max:	16 	      @:	11 
   mean:	2.8593155894 
  sigma:	2.5007943048 
    sum:	1504 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
1504
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-S.IN
#
# Empirically derived background model for the ACIS-S detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-S background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 0.000107813
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.33656e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 9.10151e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 1.41672e-05
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 1.17789e-05
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.53256e-06
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -2.72514e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 1.21828e-07
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.88227e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.01
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.574495
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 1.90619e-05
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.00301839
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = 1.90619e-05
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = 0.000594304
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.000349747
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.1
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.5
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000756713
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0345157
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.1
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.6
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.00147212
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.32209
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88427e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.63388E+04
 powll:     converged to minimum =     6.57892E+02 at iteration =      3
 powll:    final statistic value =     6.57892E+02
    bkg_mdl_c1.factor  0.0494785     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.07594E+03
 powll:     converged to minimum =     1.04245E+03 at iteration =     18
 powll:    final statistic value =     1.04245E+03
          wabs.nH  1.26383  10^22/cm^2  
            rs.kT  2.31541  keV  
            rs.norm  0.000735712  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.26383  -0.187007       +0.219884     
            rs.kT            2.31541  -0.548979       +0.829741     
            rs.norm      0.000735712  -0.000118928    +0.000130105  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.26383  -0.437199       +0.545074     
            rs.kT            2.31541  -0.853537       +2.80311      
            rs.norm      0.000735712  -0.000300771    +0.000542579  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 7.62115e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.35108730,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.49429923,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    114.969698684833,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-S.IN
#
# Empirically derived background model for the ACIS-S detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-S background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 0.000107813
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.33656e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 9.10151e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 1.41672e-05
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 1.17789e-05
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.53256e-06
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -2.72514e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 1.21828e-07
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.88227e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.01
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.574495
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 1.90619e-05
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.00301839
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = 1.90619e-05
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = 0.000594304
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.000349747
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.1
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.5
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000756713
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0345157
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.1
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.6
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.00147212
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.32209
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88427e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.63388E+04
 powll:     converged to minimum =     6.57892E+02 at iteration =      3
 powll:    final statistic value =     6.57892E+02
    bkg_mdl_c1.factor  0.0494785     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.07594E+03
 powll:     converged to minimum =     1.04245E+03 at iteration =     20
 powll:    final statistic value =     1.04245E+03
          wabs.nH  1.26181  10^22/cm^2  
            rs.kT  2.31542  keV  
            rs.norm  0.000734752  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.26181  -0.186579       +0.220833     
            rs.kT            2.31542  -0.547605       +0.833433     
            rs.norm      0.000734752  -0.000118776    +0.000129938  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.26181  -0.435185       +0.547112     
            rs.kT            2.31542  -0.853514       +2.80391      
            rs.norm      0.000734752  -0.000299784    +0.000543553  

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:55:47 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 2435.6
 LVMQT: final statistic value = 10.4812 at iteration 9
          wabs.nH  1.5806  10^22/cm^2  
            rs.kT  1.87319  keV  
            rs.norm  0.000863106  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             1.5806  -0.223281       +0.309962     
            rs.kT            1.87319  -0.401328       +0.5957       
            rs.norm      0.000863106  -0.000160906    +0.000160907  

Struct_Type[3]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH             1.5806  -0.600444       +0.808109     
            rs.kT            1.87319  -0.649657       +2.10231      
            rs.norm      0.000863106  -0.000414488    +0.000855637  

Struct_Type[3]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 6.64523e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.35108730,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.49429923,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    114.969698684833,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Fitting model c_rs2
Running sherpa --batch c_rs2.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-S.IN
#
# Empirically derived background model for the ACIS-S detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-S background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 0.000107813
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.33656e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 9.10151e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 1.41672e-05
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 1.17789e-05
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.53256e-06
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -2.72514e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 1.21828e-07
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.88227e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.01
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.574495
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 1.90619e-05
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.00301839
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = 1.90619e-05
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = 0.000594304
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.000349747
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.1
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.5
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000756713
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0345157
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.1
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.6
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.00147212
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.32209
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88427e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     1.63388E+04
 powll:     converged to minimum =     6.57892E+02 at iteration =      3
 powll:    final statistic value =     6.57892E+02
    bkg_mdl_c1.factor  0.0494785     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     3.39053E+03
 powll:     converged to minimum =     1.04246E+03 at iteration =     15
 powll:    final statistic value =     1.04246E+03
          wabs.nH  1.25382  10^22/cm^2  
            rs.kT  2.31541  keV  
            rs.norm  0.000717384  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  16.0926  keV  
           rs2.norm  1.06134e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs2.norm is equal to the rs2.norm.min limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type[3]
  run_fit()
WARNING: hit parameter space hard minimum for  rs2.kT 
WARNING: hit parameter space hard maximum for  rs2.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.25382  -0.186566       +0.219382     
            rs.kT            2.31541  -0.565204       +0.833081     
            rs.norm      0.000717384  -0.000118386    +0.000128985  
           rs2.kT            16.0926    -----           -----       
           rs2.norm      1.06134e-05  -8.36987e-05    +8.87332e-05  

Struct_Type[5]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 
WARNING: hit parameter space hard minimum for  rs2.kT 
WARNING: hit parameter space hard maximum for  rs2.kT 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.25382  -0.427752       +0.555904     
            rs.kT            2.31541  -1.20397        +2.7054       
            rs.norm      0.000717384  -0.000682192    +0.000559238  
           rs2.kT            16.0926    -----           -----       
           rs2.norm      1.06134e-05  -0.00277948     +0.00178998   

Struct_Type[5]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:56:01 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src23/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 2371.26
 LVMQT: final statistic value = 10.5111 at iteration 29
          wabs.nH  1.57935  10^22/cm^2  
            rs.kT  1.85334  keV  
            rs.norm  0.000856318  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  15.865  keV  
           rs2.norm  1.06134e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING:
   The value of rs2.norm is equal to the rs2.norm.min limit boundary.
   You may wish to consider changing min/max values and refitting.

Struct_Type
  run_fit();
WARNING: hit parameter space hard minimum for  rs2.kT 

WARNING: found better fit -- reminimizing!
 LVMQT: V2.0
 LVMQT: initial statistic value = 10.483
 LVMQT: final statistic value = 10.4812 at iteration 3
          wabs.nH  1.58084  10^22/cm^2  
            rs.kT  1.86674  keV  
            rs.norm  0.000844316  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  2.14127  keV  
           rs2.norm  1.8994e-05  10**-14 / (4 pi D**2) Int n_e n_H dV  

WARNING: hit parameter space hard minimum for  rs2.kT 
WARNING: hit parameter space hard maximum for  rs2.kT 

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH            1.58084  -0.2233         +0.309983     
            rs.kT            1.86674  -0.407022       +0.609496     
            rs.norm      0.000844316  -0.000161318    +0.000160961  
           rs2.kT            2.14127    -----           -----       
           rs2.norm       1.8994e-05  -0.00015218     +0.000152201  

Struct_Type[5]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
WARNING: upper projection bound not found for  rs.kT 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 
WARNING: hit parameter space hard minimum for  rs2.kT 
WARNING: hit parameter space hard maximum for  rs2.kT 
Projection complete for parameter: rs2.kT 
NULL
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs2"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs2.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs2.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 6.64502e-05 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.35108730,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.49429923,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    114.969698684833,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs2
Successfully updated c_rs2.mdl file
Successfully updated c_rs2.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1556' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><c_rs2.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 15:56:52> *** SUCCESS for Obsid=619  Ccdid=ACIS-S3  Srcid=23

**********************************************************************
***  Obsid=619  Srcid=24                                           ***
**********************************************************************
<2007-May-31 15:56:52> 
-----------  Process step: check_for_pause 

Processing step succeeded

-----------  Process step: get_source_lock 

Processing step succeeded

-----------  Process step: make_obsid_and_src_dirs 

Processing step succeeded

-----------  Process step: open_log_file 

Processing step succeeded

-----------  Process step: clean_files_before_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: get_resource_files 

Processing step succeeded

-----------  Process step: include_fake_processing 

Not all 'run_if' values true - skipping step

-----------  Process step: get_aspect_solution_files 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_asol1.fits
Processing step succeeded

-----------  Process step: get_event_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_evt2.fits
Processing step succeeded

-----------  Process step: get_bad_pixel_file 

Making local file /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bpix1.fits
Processing step succeeded

-----------  Process step: make_region_files 

Processing step succeeded

-----------  Process step: set_ardlib_for_bad_pixel_files 

Running acis_set_ardlib acis_bpix1.fits
Updated ardlib parameter file: /data/ANCHORS/YAXX/00619/cxcds_param_31710/ardlib.par
  AXAF_ACIS0_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bpix1.fits[BADPIX0]
  AXAF_ACIS1_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bpix1.fits[BADPIX1]
  AXAF_ACIS2_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bpix1.fits[BADPIX2]
  AXAF_ACIS3_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bpix1.fits[BADPIX3]
  AXAF_ACIS4_BADPIX_FILE -> CALDB
  AXAF_ACIS5_BADPIX_FILE -> CALDB
  AXAF_ACIS6_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bpix1.fits[BADPIX6]
  AXAF_ACIS7_BADPIX_FILE -> /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bpix1.fits[BADPIX7]
  AXAF_ACIS8_BADPIX_FILE -> CALDB
  AXAF_ACIS9_BADPIX_FILE -> CALDB
Processing step succeeded

-----------  Process step: check_for_counts_in_source 

Running test `dmlist "acis_evt2.fits[sky=region(src.reg)][energy=300:8000]" counts` -gt 1
Processing step succeeded

-----------  Process step: extract_source_spectrum 

Running psextract \
     events="acis_evt2.fits[sky=region(src.reg)]" \
     bgevents="acis_evt2.fits[sky=region(bkg.reg)]" \
     root="acis" \
     asol="acis_asol1.fits" \
     bgasol="" \
     ptype="pi" \
     gtype="NONE" \
     gspec=0 \
     clobber=yes \
     verbose=2

events=acis_evt2.fits[sky=region(src.reg)]
bgevents=acis_evt2.fits[sky=region(bkg.reg)]
root=acis
aoff=acis_asol1.fits bgaoff=acis_asol1.fits
pbkfile=NONE dafile=NONE
ptype=pi
gtype=NONE grouping=0
verbose=2

Extract source spectrum acis.pi from acis_evt2.fits[sky=region(src.reg)]
dmextract infile="acis_evt2.fits[sky=region(src.reg)][bin pi]" outfile=acis.pi opt=pha1 clobber=yes verbose=0

Extract background spectrum acis_bg.pi from acis_evt2.fits[sky=region(bkg.reg)]
dmextract infile="acis_evt2.fits[sky=region(bkg.reg)][bin pi]" outfile=acis_bg.pi opt=pha1 clobber=yes verbose=0
Inspecting events file acis_evt2.fits[sky=region(src.reg)]
Inspecting background events file acis_evt2.fits[sky=region(bkg.reg)]
Running dmstat on source and background events files:

Source Event statistics: CHIP 7 374.46993318 257.88864143 SKY 6083.3005159 4739.3497072
Background Event statistics: CHIP 7 332.33697021 212.77339488 SKY 6162.0354695 4583.639079

Look up FEF spectral calibration file(s)
Source FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=353:384,chipy=257:288]
Background FEF file is /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=321:352,chipy=193:224]
Verified Source FEF file is present
Verified background FEF file is present

Source and background FEFs are different
Building different RMFs and ARFs for source and background

Make source RMF file acis.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=353:384,chipy=257:288] outfile=acis.rmf logfile=./.psp.mlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2
Contents of mkrmf log file:

	*** mkrmf parameter inputs ***
	          input file: /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=353:384,chipy=257:288]
	         output file: acis.rmf
	        weights file: 
	               axis1: energy=0.1:11.0:0.01
	               axis2: pi=1:1024:1
	            log file: ./.psp.mlog
	               axis3: none
	               axis4: none
	               axis5: none
	           threshold: 1.00e-05
	        output formt: legacy
	clobber(1=yes, 0=no): 1
	       verbose level: 2


ATTEN:  The final MATRIX grids along "ENERGY" axis will be bound in 
		0.220000--11.000000 rather than the user-defined range 
		0.100000--11.000000.

	The final grid range of the above is to fit to FEF grid bounds, 
	but the bin size specified by user will be reduced by 12.


Created source RMF file acis.rmf

Make background RMF file acis_bg.rmf with mkrmf
mkrmf infile=/soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=321:352,chipy=193:224] outfile=acis_bg.rmf logfile=./.psp.bgmlog axis1=energy=0.1:11.0:0.01 axis2=pi=1:1024:1 clobber=yes verbose=2
mkrmf error log:

	*** mkrmf parameter inputs ***
	          input file: /soft/ciao/CALDB/data/chandra/acis/cpf/fefs/acisD2000-01-29fef_pha_ctiN0004.fits[FUNCTION][ccd_id=7,chipx=321:352,chipy=193:224]
	         output file: acis_bg.rmf
	        weights file: 
	               axis1: energy=0.1:11.0:0.01
	               axis2: pi=1:1024:1
	            log file: ./.psp.bgmlog
	               axis3: none
	               axis4: none
	               axis5: none
	           threshold: 1.00e-05
	        output formt: legacy
	clobber(1=yes, 0=no): 1
	       verbose level: 2


ATTEN:  The final MATRIX grids along "ENERGY" axis will be bound in 
		0.220000--11.000000 rather than the user-defined range 
		0.100000--11.000000.

	The final grid range of the above is to fit to FEF grid bounds, 
	but the bin size specified by user will be reduced by 12.


Created background RMF file acis_bg.rmf

Running asphist to create source aspect histogram acis.asphist
asphist infile="acis_asol1.fits" outfile=acis.asphist evtfile="acis_evt2.fits[ccd_id=7]" clobber=yes dtffile="" verbose=0
Running mkarf to create source acis.arf at (6083.3005159,4739.3497072)
mkarf detsubsys=ACIS-S3 outfile=acis.arf asphistfile="acis.asphist" sourcepixelx=6083.3005159 sourcepixely=4739.3497072 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
Running mkarf to create background acis_bg.arf at (6162.0354695,4583.639079)
mkarf detsubsys=ACIS-S3 outfile=acis_bg.arf asphistfile="acis.asphist" sourcepixelx=6162.0354695 sourcepixely=4583.639079 grating=NONE obsfile="acis_evt2.fits" pbkfile=NONE dafile=NONE maskfile=NONE verbose=0 engrid="grid(acis_bg.rmf[MATRIX][cols ENERG_LO,ENERG_HI])" clobber=yes
***ARDLIB warning: Filename acis_evt2.fits does not specify an extension. Assuming the first "interesting" extension.
No grouping selected

Group Background spectrum using BIN=1:1024:20
dmgroup infile=acis_bg.pi outfile=acis_bg_grp.pi binspec="1:1024:20" tabspec= grouptype=BIN grouptypeval= ycolumn=counts xcolumn=channel tabcolumn= clobber=yes verbose=0
Background spectrum acis_bg_grp.pi has been grouped

Updating PHA file acis.pi with BACKFILE RESPFILE ANCRFILE keys
Background spectrum (BACKFILE) = acis_bg.pi
SOURCE RMF (RESPFILE) = acis.rmf
SOURCE ARF (ANCRFILE) = acis.arf
Updating PHA file acis_bg_grp.pi with RESPFILE ANCRFILE key
BACKGROUND RMF (RESPFILE) = acis_bg.rmf
BACKGROUND ARF (ANCRFILE) = acis_bg.arf

# psextract: WARNING: For ccd_id=7 and CTI_APP=PPPPPBPBPP keyword value,
you should be using the mkacisrmf tool. The source RMF
created with mkrmf is INCORRECT for your analysis.
Run mkacisrmf independently to create a new RMF:
http://cxc.harvard.edu/ciao/threads/mkacisrmf/


# psextract: WARNING: For ccd_id=7 and CTI_APP=PPPPPBPBPP keyword value,
you should be using the mkacisrmf tool. The background RMF
created with mkrmf is INCORRECT for your analysis.
Run mkacisrmf independently to create a new RMF:
http://cxc.harvard.edu/ciao/threads/mkacisrmf/

Processing step succeeded

-----------  Process step: get_obs_info_from_pi_file 

Running dmstat
     infile=obs619/src24/acis.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	99 
    max:	20 	      @:	42 
   mean:	1.5931558935 
  sigma:	3.5894160432 
    sum:	838 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
838
Running dmstat
     infile=obs619/src24/acis_bg.pi'[channel=22:547][cols counts]'
    
COUNTS[count]
    min:	0 	      @:	34 
    max:	7 	      @:	1 
   mean:	1.4087452471 
  sigma:	1.4203302325 
    sum:	741 
   good:	526 
   null:	0 

Running pget dmstat out_sum
    
741
Processing step succeeded

-----------  Process step: make_event_image 

Processing step succeeded

-----------  Process step: fit_spectral_models 

Fitting model cstat
Running sherpa --batch cstat.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-S.IN
#
# Empirically derived background model for the ACIS-S detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-S background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 0.000107813
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.33656e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 9.10151e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 1.41672e-05
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 1.17789e-05
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.53256e-06
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -2.72514e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 1.21828e-07
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.88227e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.01
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.574495
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 1.90619e-05
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.00301839
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = 1.90619e-05
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = 0.000594304
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.000349747
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.1
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.5
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000756713
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0345157
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.1
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.6
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.00147212
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.32209
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88427e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     8.79754E+03
 powll:     converged to minimum =     5.98788E+02 at iteration =      3
 powll:    final statistic value =     5.98788E+02
    bkg_mdl_c1.factor  0.0675769     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=10
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.05202E+03
 powll:     converged to minimum =     9.10358E+02 at iteration =      6
 powll:    final statistic value =     9.10358E+02
          wabs.nH  0.0520554  10^22/cm^2  
            rs.kT  1.04365  keV  
            rs.norm  0.0027766  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0520554  -0.0121779      +0.0128638    
            rs.kT            1.04365  -0.0318255      +0.030137     
            rs.norm        0.0027766  -0.000156195    +0.000162143  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0520554  -0.0184145      +0.0198929    
            rs.kT            1.04365  -0.0375451      +0.0346455    
            rs.norm        0.0027766  -0.000248055    +0.000269335  

Struct_Type[3]
  if (1) run_proj()
  # Create postscript plot and convert to jpeg using eps2png (from yaxx/script directory)
  chips.pagewidth=6
  chips.pagelen=6
  ==> Error bars computed using Chi Gehrels.
  lplot 1 fit
  title "cstat"
  d 1 limits 0.2 10
  redraw
  print postfile cstat.ps
  ! eps2png -jpeg -width 250 -output cstat.jpg cstat.ps
  # Write fit model and header keywords to MDL file
  write mdl "cstat.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.00147335 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.33012567,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.44935324,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    807.725318129359,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store cstat
Successfully updated cstat.mdl file
Successfully updated cstat.mdl file
Fitting model c_rs
Running sherpa --batch c_rs.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-S.IN
#
# Empirically derived background model for the ACIS-S detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-S background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 0.000107813
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.33656e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 9.10151e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 1.41672e-05
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 1.17789e-05
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.53256e-06
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -2.72514e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 1.21828e-07
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.88227e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.01
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.574495
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 1.90619e-05
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.00301839
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = 1.90619e-05
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = 0.000594304
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.000349747
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.1
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.5
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000756713
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0345157
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.1
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.6
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.00147212
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.32209
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88427e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     8.79754E+03
 powll:     converged to minimum =     5.98788E+02 at iteration =      3
 powll:    final statistic value =     5.98788E+02
    bkg_mdl_c1.factor  0.0675769     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     1.05202E+03
 powll:     converged to minimum =     9.10358E+02 at iteration =      6
 powll:    final statistic value =     9.10358E+02
          wabs.nH  0.0520554  10^22/cm^2  
            rs.kT  1.04365  keV  
            rs.norm  0.0027766  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0520554  -0.0121779      +0.0128638    
            rs.kT            1.04365  -0.0318255      +0.030137     
            rs.norm        0.0027766  -0.000156195    +0.000162143  

Struct_Type[3]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0520554  -0.0184145      +0.0198929    
            rs.kT            1.04365  -0.0375451      +0.0346455    
            rs.norm        0.0027766  -0.000248055    +0.000269335  

Struct_Type[3]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:58:06 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * rs)
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 85.5192
 LVMQT: final statistic value = 75.1765 at iteration 5
          wabs.nH  0.0596173  10^22/cm^2  
            rs.kT  1.02134  keV  
            rs.norm  0.00252949  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0596173  -0.0127419      +0.014446     
            rs.kT            1.02134  -0.0353881      +0.0353832    
            rs.norm       0.00252949  -0.000152493    +0.000152493  

Struct_Type[3]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0596173  -0.0189581      +0.0217934    
            rs.kT            1.02134  -0.0438539      +0.0406397    
            rs.norm       0.00252949  -0.000242599    +0.000252222  

Struct_Type[3]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.00130011 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.33012567,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.44935324,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    807.725318129359,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs
Successfully updated c_rs.mdl file
Successfully updated c_rs.mdl file
Fitting model c_rs2
Running sherpa --batch c_rs2.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-S.IN
#
# Empirically derived background model for the ACIS-S detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-S background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 0.000107813
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.33656e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 9.10151e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 1.41672e-05
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 1.17789e-05
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.53256e-06
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -2.72514e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 1.21828e-07
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.88227e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.01
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.574495
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 1.90619e-05
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.00301839
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = 1.90619e-05
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = 0.000594304
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.000349747
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.1
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.5
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000756713
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0345157
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.1
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.6
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.00147212
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.32209
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88427e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     8.79754E+03
 powll:     converged to minimum =     5.98788E+02 at iteration =      3
 powll:    final statistic value =     5.98788E+02
    bkg_mdl_c1.factor  0.0675769     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.25692E+03
 powll:     converged to minimum =     8.88843E+02 at iteration =     17
 powll:    final statistic value =     8.88843E+02
          wabs.nH  0.0499035  10^22/cm^2  
            rs.kT  1.99724  keV  
            rs.norm  0.00140639  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.856053  keV  
           rs2.norm  0.00127103  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0499035  -0.0121819      +0.0128688    
            rs.kT            1.99724  -0.415263       +0.712089     
            rs.norm       0.00140639  -0.000168173    +0.000175585  
           rs2.kT           0.856053  -0.0313759      +0.0291599    
           rs2.norm       0.00127103  -0.00012149     +0.000126643  

Struct_Type[5]
  if (1) run_unc()
Projection: optimization reset to Simplex.
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0499035  -0.019737       +0.0213172    
            rs.kT            1.99724  -3.04711        +1.17284      
            rs.norm       0.00140639  -0.000421021    +0.000505745  
           rs2.kT           0.856053  -0.0689004      +0.0403199    
           rs2.norm       0.00127103  -0.000392408    +0.000366576  

Struct_Type[5]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:58:16 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  source = (wabs * (rs+rs2))
  rs.kT.max=50
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 70.788
 LVMQT: final statistic value = 58.3243 at iteration 5
          wabs.nH  0.0624745  10^22/cm^2  
            rs.kT  1.89504  keV  
            rs.norm  0.0012468  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.855223  keV  
           rs2.norm  0.00130862  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0624745  -0.0127932      +0.0144397    
            rs.kT            1.89504  -0.424234       +0.709534     
            rs.norm        0.0012468  -0.000172787    +0.000172784  
           rs2.kT           0.855223  -0.0287992      +0.0287994    
           rs2.norm       0.00130862  -0.000125615    +0.000125616  

Struct_Type[5]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.norm 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH          0.0624745  -0.020196       +0.0227183    
            rs.kT            1.89504  -0.515864       +1.13696      
            rs.norm        0.0012468  -0.000415733    +0.00133876   
           rs2.kT           0.855223  -0.0656478      +0.0387277    
           rs2.norm       0.00130862  -0.000391828    +0.000358027  

Struct_Type[5]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs2"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs2.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs2.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.00134384 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.33012567,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.44935324,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    807.725318129359,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs2
Successfully updated c_rs2.mdl file
Successfully updated c_rs2.mdl file
Fitting model c_rs2a
Running sherpa --batch c_rs2a.in
    
    Abundances set to Anders & Grevesse
Echo is on
  echo on
Model parameter prompting is off
  paramprompt off
1
  evalfile("sherpa_plotfns.sl")
  require("fits")
  require("sherpa_utils")
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.arf
  data acis.pi
  ignore energy :0.3,8:
  statistic cstat
  method powell
# ACIS-S.IN
#
# Empirically derived background model for the ACIS-S detector, based on
# fitting an 8th order polynomial plus 6 gaussians to ACIS-S background
# data.  Issues about time-dependent QE degradation etc are murky, but this
# background should be useful in the low-counts/high-background case to
# improve fit accuracy.
#
notice back energy 0.5:8
poly1d[bkg_mdl_p1]
gauss1d[bkg_mdl_g1]
gauss1d[bkg_mdl_g2]
gauss1d[bkg_mdl_g3]
gauss1d[bkg_mdl_g4]
gauss1d[bkg_mdl_g5]
gauss1d[bkg_mdl_g6]
xsconstant[bkg_mdl_c1]
bkg_mdl_c1.factor = 1e-4
thaw bkg_mdl_c1
bkg_mdl_p1 integrate on
bkg_mdl_p1.c0.min = -6.41459e-05
bkg_mdl_p1.c0.max = 0.00190619
bkg_mdl_p1.c0.value = 0.000107813
bkg_mdl_p1.c0.type = freeze
bkg_mdl_p1.c1.min = -0.0192035
bkg_mdl_p1.c1.max = 0.0192035
bkg_mdl_p1.c1.value = 2.33656e-05
bkg_mdl_p1.c1.type = freeze
bkg_mdl_p1.c2.min = -0.002002
bkg_mdl_p1.c2.max = 0.002002
bkg_mdl_p1.c2.value = 9.10151e-06
bkg_mdl_p1.c2.type = freeze
bkg_mdl_p1.c3.min = -6.41459e-05
bkg_mdl_p1.c3.max = 0.00190619
bkg_mdl_p1.c3.value = 1.41672e-05
bkg_mdl_p1.c3.type = freeze
bkg_mdl_p1.c4.min = -6.41459e-05
bkg_mdl_p1.c4.max = 0.00190619
bkg_mdl_p1.c4.value = 1.17789e-05
bkg_mdl_p1.c4.type = freeze
bkg_mdl_p1.c5.min = -6.41459e-05
bkg_mdl_p1.c5.max = 0.00190619
bkg_mdl_p1.c5.value = 1.53256e-06
bkg_mdl_p1.c5.type = freeze
bkg_mdl_p1.c6.min = -6.41459e-05
bkg_mdl_p1.c6.max = 0.00190619
bkg_mdl_p1.c6.value = -2.72514e-07
bkg_mdl_p1.c6.type = freeze
bkg_mdl_p1.c7.min = -6.41459e-05
bkg_mdl_p1.c7.max = 0.00190619
bkg_mdl_p1.c7.value = 1.21828e-07
bkg_mdl_p1.c7.type = freeze
bkg_mdl_p1.c8.min = -6.41459e-05
bkg_mdl_p1.c8.max = 0.00190619
bkg_mdl_p1.c8.value = 3.88227e-08
bkg_mdl_p1.c8.type = freeze
bkg_mdl_p1.offset.min = -0.4015
bkg_mdl_p1.offset.max = 9.9937
bkg_mdl_p1.offset.value = 5
bkg_mdl_p1.offset.type = freeze
bkg_mdl_g1 integrate on
bkg_mdl_g1.fwhm.min = 0.001
bkg_mdl_g1.fwhm.max = 345.157
bkg_mdl_g1.fwhm.value = 0.01
bkg_mdl_g1.fwhm.type = freeze
bkg_mdl_g1.pos.min = 0.4015
bkg_mdl_g1.pos.max = 9.9937
bkg_mdl_g1.pos.value = 0.574495
bkg_mdl_g1.pos.type = freeze
bkg_mdl_g1.ampl.min = 1.90619e-05
bkg_mdl_g1.ampl.max = 0.190619
bkg_mdl_g1.ampl.value = 0.00301839
bkg_mdl_g1.ampl.type = freeze
bkg_mdl_g2 integrate on
bkg_mdl_g2.fwhm.min = 0.01
bkg_mdl_g2.fwhm.max = 345.157
bkg_mdl_g2.fwhm.value = 0.0317183
bkg_mdl_g2.fwhm.type = freeze
bkg_mdl_g2.pos.min = 0.4015
bkg_mdl_g2.pos.max = 9.9937
bkg_mdl_g2.pos.value = 1.7752
bkg_mdl_g2.pos.type = freeze
bkg_mdl_g2.ampl.min = 1.90619e-05
bkg_mdl_g2.ampl.max = 0.190619
bkg_mdl_g2.ampl.value = 0.000594304
bkg_mdl_g2.ampl.type = freeze
bkg_mdl_g3 integrate on
bkg_mdl_g3.fwhm.min = 0.0345157
bkg_mdl_g3.fwhm.max = 345.157
bkg_mdl_g3.fwhm.value = 0.0864722
bkg_mdl_g3.fwhm.type = freeze
bkg_mdl_g3.pos.min = 0.4015
bkg_mdl_g3.pos.max = 9.9937
bkg_mdl_g3.pos.value = 2.15107
bkg_mdl_g3.pos.type = freeze
bkg_mdl_g3.ampl.min = 1.90619e-05
bkg_mdl_g3.ampl.max = 0.190619
bkg_mdl_g3.ampl.value = 0.000349747
bkg_mdl_g3.ampl.type = freeze
bkg_mdl_g4 integrate on
bkg_mdl_g4.fwhm.min = 0.0345157
bkg_mdl_g4.fwhm.max = 345.157
bkg_mdl_g4.fwhm.value = 0.1
bkg_mdl_g4.fwhm.type = freeze
bkg_mdl_g4.pos.min = 0.4015
bkg_mdl_g4.pos.max = 9.9937
bkg_mdl_g4.pos.value = 7.5
bkg_mdl_g4.pos.type = freeze
bkg_mdl_g4.ampl.min = 1.90619e-05
bkg_mdl_g4.ampl.max = 0.190619
bkg_mdl_g4.ampl.value = 0.000756713
bkg_mdl_g4.ampl.type = freeze
bkg_mdl_g5 integrate on
bkg_mdl_g5.fwhm.min = 0.0345157
bkg_mdl_g5.fwhm.max = 345.157
bkg_mdl_g5.fwhm.value = 0.1
bkg_mdl_g5.fwhm.type = freeze
bkg_mdl_g5.pos.min = 0.4015
bkg_mdl_g5.pos.max = 9.9937
bkg_mdl_g5.pos.value = 9.6
bkg_mdl_g5.pos.type = freeze
bkg_mdl_g5.ampl.min = 1.90619e-05
bkg_mdl_g5.ampl.max = 0.190619
bkg_mdl_g5.ampl.value = 0.00147212
bkg_mdl_g5.ampl.type = freeze
bkg_mdl_g6 integrate on
bkg_mdl_g6.fwhm.min = 0.0345157
bkg_mdl_g6.fwhm.max = 345.157
bkg_mdl_g6.fwhm.value = 0.180799
bkg_mdl_g6.fwhm.type = freeze
bkg_mdl_g6.pos.min = 0.4015
bkg_mdl_g6.pos.max = 9.9937
bkg_mdl_g6.pos.value = 1.32209
bkg_mdl_g6.pos.type = freeze
bkg_mdl_g6.ampl.min = 0
bkg_mdl_g6.ampl.max = 0.190619
bkg_mdl_g6.ampl.value = 1.88427e-05
bkg_mdl_g6.ampl.type = freeze
background = bkg_mdl_c1 * (bkg_mdl_p1 + bkg_mdl_g1 + bkg_mdl_g2 + bkg_mdl_g3 + bkg_mdl_g4 + bkg_mdl_g5 + bkg_mdl_g6)
 powll: v1.2
 powll:  initial statistic value =     8.79754E+03
 powll:     converged to minimum =     5.98788E+02 at iteration =      3
 powll:    final statistic value =     5.98788E+02
    bkg_mdl_c1.factor  0.0675769     

bfit
freeze bkg_mdl_c1
  xswabs[wabs]
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  rs.Abundanc.type=thaw
  rs2.Abundanc.type=thaw
  rs2.Abundanc => rs.Abundanc
  rs.kT.max=50
  source = (wabs * (rs+rs2))
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 powll: v1.2
 powll:  initial statistic value =     2.25692E+03
 powll:     converged to minimum =     8.92823E+02 at iteration =     31
 powll:    final statistic value =     8.92823E+02
          wabs.nH  0.116533  10^22/cm^2  
            rs.kT  1.0243  keV  
            rs.Abundanc  0.147775     
            rs.norm  0.00396923  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.280162  keV  
           rs2.norm  0.00109622  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type[3]
  run_fit()

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.116533  -0.0131303      +0.0137442    
            rs.kT             1.0243  -0.0510956      +0.0496667    
            rs.Abundanc     0.147775  -0.018493       +0.0191634    
            rs.norm       0.00396923  -0.00025649     +0.000265238  
           rs2.kT           0.280162  -0.0518828      +0.064207     
           rs2.norm       0.00109622  -0.000337044    +0.000356782  

Struct_Type[6]
  if (1) run_unc()
Projection: optimization reset to Simplex.
WARNING: lower projection bound not found for  wabs.nH 
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.Abundanc 
Projection complete for parameter: rs.norm 
WARNING: upper projection bound not found for  rs2.kT 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.116533  -0.116533       +0.0495535    
            rs.kT             1.0243  -0.0936235      +0.080597     
            rs.Abundanc     0.147775  -0.0677249      +0.10765      
            rs.norm       0.00396923  -0.00309158     +0.00133768   
           rs2.kT           0.280162  -0.0820089      +63.7198      
           rs2.norm       0.00109622  -0.000808042    +0.00192966   

Struct_Type[6]
  if (1) run_proj()
#------------------------------------------------------------------
# Fit a grouped PHA or PI spectrum in Sherpa
# 
# This sherpa script automatically created by yaxx on Thu May 31 15:58:59 2007
#------------------------------------------------------------------
The inferred file type is PHA.  If this is not what you want, please 
specify the type explicitly in the data command.
Background data are being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis_bg.pi
RMF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.rmf
ARF is being input from:
  /data/ANCHORS/YAXX/00619/Data/obs619/src24/acis.arf
  data acis.pi
WARNING: any applied filters are being deleted!
  groupByCounts(8)
  subtract
  ignore energy :0.3,8:
  statistic chi dvar
  method levenberg-marquardt
  xswabs[wabs]
Error: model component name wabs is already in use.
       If the last command was to use wabs in a model stack,
       that stack has been deleted.
    wabs.nh       = 0.1
    wabs.nh.min=1e-4
    wabs.nh.max=100
    xsraymond[rs]
Error: model component name rs is already in use.
       If the last command was to use rs in a model stack,
       that stack has been deleted.
    rs.kT.min = 0.01
    rs.kT.max = 50
    rs.Abundanc.value = 0.3
    rs.Abundanc.type = freeze
    xsraymond[rs2]
Error: model component name rs2 is already in use.
       If the last command was to use rs2 in a model stack,
       that stack has been deleted.
    rs2.kT.min = 0.01
    rs2.kT.max = 50
    rs2.Abundanc.value = 0.3
    rs2.Abundanc.type = freeze
  rs.Abundanc.type=thaw
  rs2.Abundanc.type=thaw
  rs2.Abundanc => rs.Abundanc
  rs.kT.max=50
  source = (wabs * (rs+rs2))
  sherpa.proj.sigma = 1.6
  sherpa.unc.sigma = 1.6
 LVMQT: V2.0
 LVMQT: initial statistic value = 359.327
 LVMQT: final statistic value = 56.097 at iteration 5
          wabs.nH  0.144614  10^22/cm^2  
            rs.kT  0.983977  keV  
            rs.Abundanc  0.151937     
            rs.norm  0.00376508  10**-14 / (4 pi D**2) Int n_e n_H dV  
           rs2.kT  0.248504  keV  
           rs2.norm  0.00166827  10**-14 / (4 pi D**2) Int n_e n_H dV  

Struct_Type
  run_fit();

Computed for sherpa.unc.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.144614  -0.0138092      +0.0153057    
            rs.kT           0.983977  -0.0580536      +0.0579235    
            rs.Abundanc     0.151937  -0.0181873      +0.0181312    
            rs.norm       0.00376508  -0.000264825    +0.000265425  
           rs2.kT           0.248504  -0.0390942      +0.0401455    
           rs2.norm       0.00166827  -0.000437708    +0.000437841  

Struct_Type[6]
  if (1) run_unc()
Projection complete for parameter: wabs.nH 
Projection complete for parameter: rs.kT 
Projection complete for parameter: rs.Abundanc 
Projection complete for parameter: rs.norm 
Projection complete for parameter: rs2.kT 
Projection complete for parameter: rs2.norm 

Computed for sherpa.proj.sigma = 1.6
        --------------------------------------------------------
        Parameter Name      Best-Fit Lower Bound     Upper Bound
        --------------------------------------------------------
          wabs.nH           0.144614  -0.0501538      +0.0817143    
            rs.kT           0.983977  -0.117009       +0.0946696    
            rs.Abundanc     0.151937  -0.0745599      +0.127156     
            rs.norm       0.00376508  -0.00112445     +0.00162399   
           rs2.kT           0.248504  -0.064339       +0.126872     
           rs2.norm       0.00166827  -0.00112595     +0.00455243   

Struct_Type[6]
  if (1) run_proj()
  set_log()
Warning: negative and zero values ignored in log scale
Warning: negative and zero values ignored in log scale
  lplot 2 fit delchi
  title "c\_rs2a"
  d 1 limits 0.2 10
  d 2 limits 0.2 10
  redraw
  print postfile c_rs2a.ps
  # Write fit model and header keywords to MDL file
  write mdl "c_rs2a.mdl"
  # Get the model flux in the specified energy range and fit statistics
Flux for source dataset 1: 0.00126348 photons/cm**2/s
  flux = get_eflux(1, [0.3, 8])
  flux = get_eflux(1, [0.3, 8])
  # Open MDL_Models block of MDL file		      
  # Write important values as MDL file header keywords
  fits_update_key (fp, "RA",        246.33012567,       "Right Ascension")
  fits_update_key (fp, "DEC",       -24.44935324,      "Declination")
  fits_update_key (fp, "OBJECT",   "OPHIUCHI MOSAIC #2",  "Object name")
  fits_update_key (fp, "COUNTS",    807.725318129359,   "Counts")
  fits_update_key (fp, "EXPOSURE",  4.1199614976785E+03, "Exposure time (sec)")
  fits_update_key (fp, "EFLUX",      flux.value,        "Flux (" + flux.units + ")")
  fits_update_key (fp, "EFLUX1",      flux_dekt1.value,        "Unabs. Flux kT1 (" + flux_dekt1.units + ")")
  fits_update_key (fp, "EFLUX2",      flux_dekt2.value,        "Unabs. Flux kT2 (" + flux_dekt2.units + ")")
  fits_update_key (fp, "F_METHOD",  get_method_expr(), "Fit method name")
  fits_update_key (fp, "F_STATNM",  get_stat_expr(),   "Fit statistic name")
  fits_update_key (fp, "F_DOF",     fit_stat[0].dof,   "Fit degrees of freedom")
  fits_update_key (fp, "F_STAT",    fit_stat[0].stat,  "Fit statistic")
  fits_update_key (fp, "F_NUMBIN",  fit_stat[0].numbins, "Fit number of bins")
  if (fit_stat[0].rstat != NULL) fits_update_key (fp, "F_RSTAT", fit_stat[0].rstat, "Fit reduced statistic")
  if (fit_stat[0].qval  != NULL) fits_update_key (fp, "F_QVAL",  fit_stat[0].qval,  "Fit q-value (probability)")
  # Close file
  fits_close_file (fp)
  store c_rs2a
Successfully updated c_rs2a.mdl file
Successfully updated c_rs2a.mdl file
Processing step succeeded

-----------  Process step: make_latex_report 

Making LaTeX report
Running latex -interaction=batchmode report.tex
    
This is pdfeTeX, Version 3.141592-1.21a-2.2 (Web2C 7.5.4)
entering extended mode
Running dvips report -o
    
This is dvips(k) 5.95a Copyright 2005 Radical Eye Software (www.radicaleye.com)
' TeX output 2007.05.31:1600' -> report.ps
<tex.pro><texps.pro><special.pro><color.pro>. <cmsy8.pfb><cmmi8.pfb>
<cmr8.pfb><cmr12.pfb><cmbx12.pfb>[1
dvips: Could not find figure file image.ps; continuing
<c_rs.ps><c_rs2.ps><c_rs2a.ps><cstat.ps>] 
Processing step succeeded

-----------  Process step: make_html_report 

Making HTML report
Processing step succeeded

-----------  Process step: store_source_information 

Processing step succeeded

-----------  Process step: clean_files_after_processing 

Not all 'run_if' values defined - skipping step

-----------  Process step: release_source_lock 

Processing step succeeded
<2007-May-31 16:00:52> *** SUCCESS for Obsid=619  Ccdid=ACIS-S3  Srcid=24

Creating HTML report index
Can't remove directory /data/ANCHORS/YAXX/00619/cxcds_param_31710: Directory not empty at /data/ANCHORS/YAXX/bin/yaxx-0.908-linux/yaxx-perl/IO/All/Dir.pm line 181
ANCHORS: Running Post-YAXX Processing
run_dmextract.pl /data/ANCHORS/YAXX/00619/sample.rdb 619 evt2_efiltbin4_expmap.fits
run_dmcopy.pl /data/ANCHORS/YAXX/00619/sample.rdb 619 evt2_efiltbin4_expmap.fits
run_bblocks.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
Chips Error: ;
run_gl.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
run_quantile.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
IDL Version 6.3 (linux x86 m32). (c) 2006, Research Systems, Inc.
Installation number: 209295.
Licensed for use by: Smithsonian Astrophysical Observatory

% Compiled module: BBLOCKS_PLOT.
% Compiled module: READCOL.
% Compiled module: NUMLINES.
% Compiled module: OS_FAMILY.
% Compiled module: TAG_EXIST.
% Compiled module: DATATYPE.
% Compiled module: ZPARCHECK.
% Compiled module: REMCHAR.
% Compiled module: GETTOK.
% Compiled module: REPCHR.
% Compiled module: STRNUMBER.
% READCOL: 24 valid lines read
% Compiled module: LOADCT.
% Unsupported X Windows visual (class: DirectColor, depth: 24).
  Substituting default (class: TrueColor, Depth: 24).
% Compiled module: FILEPATH.
% Compiled module: PATH_SEP.
% LOADCT: Loading table Rainbow + white
% Compiled module: STRSPLIT.
% Compiled module: MRDFITS.
% Compiled module: FXPOSIT.
% Compiled module: MRD_HREAD.
% Compiled module: FXPAR.
% Compiled module: VALID_NUM.
% Compiled module: MRD_SKIP.
% Compiled module: MRD_STRUCT.
% Compiled module: IS_IEEE_BIG.
% Compiled module: IEEE_TO_HOST.
% Compiled module: WRITE_GIF.
% Loaded DLM: GIF.
% Compiled module: SPECTRA_PLOT.
% READCOL: 24 valid lines read
% LOADCT: Loading table Rainbow + white
% Compiled module: ERRPLOT.
% Attempt to call undefined procedure/function: 'GLVARY_PLOT'.
% Execution halted at: $MAIN$          
collect_skyview.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
collect_img_to_jpg.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
run_2mass.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
--16:15:20--  http://irsa.ipac.caltech.edu/cgi-bin/Oasis/CatSearch/nph-catsearch?server=%40rmt_stone&database=fp_2mass&catalog=fp_psc&sql=select+ra%2C+dec%2C+j_m%2Cj_cmsig%2Cj_msigcom%2Ch_m%2Ch_cmsig%2Ch_msigcom%2Ck_m%2Ck_cmsig%2Ck_msigcom%2Cph_qual%2Crd_flg%2Cbl_flg%2Ccc_flg%2Cgal_contam%2Cmp_flg%2Cprox%2Cpxpa+from+fp_psc&within=12+arcmin&objstr=246.6282689473+-24.5379384717
Resolving irsa.ipac.caltech.edu... 134.4.10.120
Connecting to irsa.ipac.caltech.edu|134.4.10.120|:80... connected.
HTTP request sent, awaiting response... 200 OK
Length: unspecified [text/plain]
Saving to: `/data/ANCHORS/YAXX/00619/fp_2mass_tmp.tbl'

     0K .......... .......... .......... .......... ..........  181K
    50K .......... ....                                         156K=0.4s

16:15:29 (175 KB/s) - `/data/ANCHORS/YAXX/00619/fp_2mass_tmp.tbl' saved [65616]

IDL Version 6.3 (linux x86 m32). (c) 2006, Research Systems, Inc.
Installation number: 209295.
Licensed for use by: Smithsonian Astrophysical Observatory

% Compiled module: MATCH_OBSID.
% Compiled module: READCOL.
% Compiled module: NUMLINES.
% Compiled module: OS_FAMILY.
% Compiled module: TAG_EXIST.
% Compiled module: DATATYPE.
% Compiled module: ZPARCHECK.
% Compiled module: REMCHAR.
% Compiled module: GETTOK.
% Compiled module: REPCHR.
% Compiled module: STRNUMBER.
% READCOL: 24 valid lines read
% READCOL: 395 valid lines read
% Compiled module: GCIRC.
% Compiled module: ISARRAY.
collect_target_table.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
assemble_report.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs2a.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs2a.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
Cannot open c_rs.ps
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs2.ps
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
Cannot open c_rs2a.ps
warning: failed to load external entity "/tmp/2mass.xml"
merge2web.pl /data/ANCHORS/YAXX/00619/sample.rdb 619
rsync: link_stat "/data/ANCHORS/YAXX/00619/Data/obs619/../../LOG/*" failed: No such file or directory (2)
rsync error: some files could not be transferred (code 23) at main.c(977) [sender=2.6.9]