Each identified distinct X-ray source on the sky is
represented in the catalog by one or more
"source observation" entries - one
for each observation in which the source has been detected - and a
single "master
source" entry. The individual source entries record all of the
properties about a detection extracted from a single
observation, as well as associated
file-based data
products, which are observation-specific.
| Context |
Column Name |
Type |
Units |
Description |
|
Observation Identification
|
obsid |
integer |
|
Observation Id (ObsID)
|
| obi |
integer |
|
Observation Interval (ObI)
|
|
|
Pointing Information
|
targname |
string |
|
target name for the observation
|
| ra_targ |
double |
deg |
ICRS right ascension of
the target
|
| dec_targ |
double |
deg |
ICRS declination of the
target
|
| ra_pnt |
double |
deg |
ICRS right ascension of
the mean pointing
|
| dec_pnt |
double |
deg |
ICRS declination of the
mean pointing
|
| roll_pnt |
double |
deg |
roll angle of the mean pointing
|
| ra_nom |
double |
deg |
ICRS right ascension of
the tangent point
|
| dec_nom |
double |
deg |
ICRS declination of the
tangent point
|
| roll_nom |
double |
deg |
roll angle of the tangent point
|
|
|
Timing Information
|
gti_start |
double |
s |
start time for the
valid data
in mission elapsed time
|
| gti_stop |
double |
s |
stop time for the
valid data in
mission elapsed time
|
| gti_elapse |
double |
s |
total elapsed time of the observation. The total elapsed
time is not equal to the total exposure time of the
observation because periods of bad time may have been
filtered out.
|
| gti_obs |
string |
|
start time for the
valid data in
FITS standard format (ISO 8601)
|
| gti_end |
string |
|
stop time for the
valid data in
FITS standard format (ISO 8601)
|
| gti_mjd_obs |
double |
|
modified Julian date for the start time of the
valid data
|
| mjd_ref |
double |
|
modified Julian date reference corresponding to zero
seconds mission elapsed time
|
|
|
Instrument Information
|
instrument |
string |
|
instrument used for the observation: ACIS or HRC
|
| grating |
string |
|
grating used for the observation: NONE, HETG, or LETG
|
| datamode |
string |
|
data mode used for the observation
|
| readmode |
string |
|
readout mode used for the observation: TIMED or
CONTINUOUS; ACIS only
|
| cycle |
string |
|
cycle for alternating exposure
(interleaved) mode observations: P (primary) or
S (secondary); ACIS only. Value is P for full-frame
observations.
|
| exptime |
double |
|
CCD frame time; ACIS only
|
| timing_mode |
boolean |
|
TRUE if the observation was done in precision timing mode,
FALSE if not; HRC only
|
|
|
Processing Information
|
ascdsver |
string |
|
software version used to create the Level 3 event file
|
| caldbver |
string |
|
calibration database version used to create the Level 3
event file
|
| crdate |
string |
|
creation date and time (UTC) of the Level 3 event file
|
|
|
Observing Cycle
|
ao |
integer |
|
Announcement of Opportunity (AO) number for the Chandra
observing cycle in which the observation was scheduled
|
|
|
Source Identification
|
region_id |
integer |
|
source region within the observation
|
| source_id |
integer |
|
source component within the source region. For the first
catalog release, this is always "1".
|
|
|
Position and Position Errors
|
ra |
double[6] |
deg |
ICRS right ascension of
the source for each science energy band
|
| dec |
double[6] |
deg |
ICRS declination of the
source for each science energy band
|
| err_ellipse_r0 |
double[6] |
arcsec |
major radius of the 95% confidence
level error ellipse of the source position for each science energy band
|
| err_ellipse_r1 |
double[6] |
arcsec |
minor radius of the 95% confidence level error ellipse of the source
position for each science energy band
|
| err_ellipse_ang |
double[6] |
deg |
position angle of the major axis of the
95% confidence level error
ellipse of the source position for each science energy band
|
| gal_l |
double[6] |
deg |
Galactic longitude of the source for each science energy band for equinox
J2000.0 and epoch J2000.0
|
| gal_b |
double[6] |
deg |
Galactic latitude of the source for each science energy band for equinox
J2000.0 and epoch J2000.0
|
| theta |
double |
arcmin |
off-axis angle, θ, of the source
|
| phi |
double |
deg |
azimuthal angle, φ, of the source
|
| chipx |
double |
pixel |
the chipx position corresponding to the off-axis angles
(θ, φ) of the source
|
| chipy |
double |
pixel |
the chipy position corresponding to the off-axis angles
(θ, φ) of the source
|
|
|
Source Significance
|
detect_significance |
double[6] |
|
source significance of the detection computed by
wavdetect for each source detection energy band
|
| flux_significance |
double[6] |
|
flux significance for each source detection energy band
|
|
|
Source Flags
|
extent_code |
coded byte |
|
indicates whether the source is extended in all science energy bands
|
| conf_code |
coded byte |
|
indicates whether the source is in a confused region in any
source detection energy band
|
| pileup_warning |
double |
|
indicates that the source properties may be affected by ACIS
pileup
|
| var_code |
coded byte |
|
indicates source variability in any science energy band
|
| edge_code |
coded byte |
|
indicates that the position or region dithered off a chip
boundary
|
| multi_chip_code |
coded byte |
|
indicates that the position or region dithered over multiple
chip boundaries
|
| streak_src_flag |
boolean |
|
indicates that the source lies on an ACIS readout streak
|
| sat_src_flag |
boolean |
|
indicates a saturated source (strong ACIS pileup)
|
| man_inc_flag |
boolean |
|
indicates the source was identified manually (automatic
detection failed)
|
| man_reg_flag |
boolean |
|
indicates that source parameters were manually adjusted due
to pileup
|
|
|
Source Extent and Errors
|
ra_aper |
double |
deg |
ICRS right ascension of
the center of the source and
background regions
|
| dec_aper |
double |
deg |
ICRS declination of the
center of the source and background regions
|
| mjr_axis_aper |
double |
arcsec |
semi-major axis of the source region ellipse
|
| mnr_axis_aper |
double |
arcsec |
semi-minor axis of the source region ellipse
|
| pos_angle_aper |
double |
deg |
position angle of the semi-major axis of the source region
ellipse
|
| mjr_axis1_aperbkg |
double |
arcsec |
semi-major axis of the inner background annulus ellipse
|
| mnr_axis1_aperbkg |
double |
arcsec |
semi-minor axis of the inner background annulus ellipse
|
| mjr_axis2_aperbkg |
double |
arcsec |
semi-major axis of the outer background annulus ellipse
|
| mnr_axis2_aperbkg |
double |
arcsec |
semi-minor axis of the outer background annulus ellipse
|
| pos_angle_aperbkg |
double |
deg |
position angle of the inner and outer semi-major axes of the
background annulus ellipse
|
| area_aper |
double |
sq. arcseconds |
area of the modified source region
|
| area_aperbkg |
double |
sq. arcseconds |
area of the modified background region
|
| mjr_axis_raw |
double[6] |
arcsec |
1σ radius along the major axis of the rotated elliptical Gaussian
parameterization of the raw extent of a source for each science energy band
|
| mnr_axis_raw |
double[6] |
arcsec |
1σ radius along the minor axis of the rotated elliptical Gaussian
parameterization of the raw extent of a source for each science energy band
|
| pos_angle_raw |
double[6] |
deg |
position angle of the rotated elliptical Gaussian
parameterization of the raw extent of a source for each science energy band
|
| mjr_axis_raw_err |
double[6] |
arcsec |
error on the "mjr_axis_raw" value for each science energy band
|
| mnr_axis_raw_err |
double[6] |
arcsec |
error on the "mnr_axis_raw" value for each science energy band
|
| pos_angle_raw_err |
double[6] |
deg |
error on the "pos_angle_raw" value for each science energy band
|
| psf_mjr_axis_raw |
double[6] |
arcsec |
major axis of the rotated elliptical Gaussian
parameterization of the raw extent of the
PSF for each science energy band
|
| psf_mnr_axis_raw |
double[6] |
arcsec |
minor axis of the rotated elliptical Gaussian
parameterization of the raw extent of the
PSF for each science energy band
|
| psf_pos_angle_raw |
double[6] |
deg |
position angle of the rotated elliptical Gaussian
parameterization of the raw extent of the
PSF for each science energy band
|
| psf_mjr_axis_raw_err |
double[6] |
arcsec |
error on the "psf_mjr_axis_raw" value for each science energy band
|
| psf_mnr_axis_raw_err |
double[6] |
arcsec |
error on the "psf_mnr_axis_raw" value for each science energy band
|
| psf_pos_angle_raw_err |
double[6] |
arcsec |
error on the "psf_pos_angle_raw" value for each science energy band
|
| major_axis |
double[6] |
arcsec |
best estimate value for the 1σ radius along the major
axis of the rotated elliptical Gaussian
parameterization of the deconvolved
source extent ellipse for each science energy band
|
| minor_axis |
double[6] |
arcsec |
best estimate value for 1σ radius along the minor axis
of the rotated
elliptical Gaussian parameterization of the deconvolved
source extent ellipse for each science energy band
|
| pos_angle |
double[6] |
deg |
best estimate value for the position angle of the rotated
elliptical Gaussian parameterization of the deconvolved
source extent ellipse for each science energy band
|
| major_axis_err |
double[6] |
arcsec |
error on the "major_axis" value for each science energy band
|
| minor_axis_err |
double[6] |
arcsec |
error on the "minor_axis" value for each science energy band
|
| pos_angle_err |
double[6] |
deg |
error on the "pos_angle" value for each science energy band
|
|
|
Source Fluxes
|
cnts_aper |
long[6] |
counts |
total counts measured in the modified source region for each science energy band
|
| cnts_aperbkg |
long[6] |
counts |
total counts measured in the modified background region for each science energy band
|
| cnts_aper90 |
long[6] |
counts |
total counts measured in the modified elliptical aperture for each science energy band
|
| cnts_aper90bkg |
long[6] |
counts |
total counts measured in the modified elliptical background
aperture for each science energy band
|
| src_cnts_aper |
double[6] |
counts |
net background-subtracted source counts inferred from the
modified source region for each science energy band
|
| src_cnts_aper90 |
double[6] |
counts |
net background-subtracted source counts inferred from the
modified
elliptical aperture for each science energy band
|
| mjr_axis_aper90 |
double |
arcsec |
major axis of the elliptical aperture that contains the 90%
Encircled Counts Fraction of the PSF at the source location
|
| mnr_axis_aper90 |
double |
arcsec |
minor axis of the elliptical aperture that contains the 90%
Encircled Counts Fraction of the PSF at the source location
|
| pos_angle_aper90 |
double |
deg |
position angle of the elliptical aperture that contains the
90% Encircled Counts Fraction of the PSF at the source location
|
| mjr_axis1_aper90bkg |
double |
arcsec |
major axis of the inner annulus of the co-located, scaled
elliptical background aperture
|
| mnr_axis1_aper90bkg |
double |
arcsec |
minor axis of the inner annulus of the co-located, scaled
elliptical background aperture
|
| mjr_axis2_aper90bkg |
double |
arcsec |
major axis of the outer annulus of the co-located, scaled
elliptical background aperture
|
| mnr_axis2_aper90bkg |
double |
arcsec |
minor axis of the outer annulus of the co-located, scaled
elliptical background aperture
|
| pos_angle_aper90bkg |
double |
deg |
position angle of the co-located, scaled
elliptical background aperture
|
| area_aper90 |
double[6] |
sq. arcseconds |
area of the modified elliptical aperture
|
| area_aper90bkg |
double[6] |
sq. arcseconds |
area of the modified elliptical background aperture
|
| src_rate_aper |
double[6] |
Hz |
background-subtracted source count rate inferred from the
modified source region for each science energy band
|
| src_rate_aper_hilim |
double[6] |
Hz |
upper limit on the confidence interval of the
"src_rate_aper" value for each science energy band
|
| src_rate_aper_lolim |
double[6] |
Hz |
lower limit on the confidence interval of the
"src_rate_aper" value for each science energy band
|
| src_rate_aper90 |
double[6] |
Hz |
background-subtracted source count rate inferred from the
modified elliptical aperture for each science energy band
|
| src_rate_aper90_hilim |
double[6] |
Hz |
upper limit on the confidence interval of the
"src_rate_aper90" value for each science energy band
|
| src_rate_aper90_lolim |
double[6] |
Hz |
lower limit on the confidence interval of the
"src_rate_aper90" value for each science energy band
|
| photflux_aper |
double[6] |
photons s-1 cm-2
|
background-subtracted flux inferred from the modified source region for each science energy band
|
| photflux_aper_hilim |
double[6] |
photons s-1 cm-2
|
upper limit on the confidence interval of the
"photflux_aper" value for each science energy band
|
| photflux_aper_lolim |
double[6] |
photons s-1 cm-2
|
lower limit on the confidence interval of the
"photflux_aper" value for each science energy band
|
| photflux_aper90 |
double[6] |
photons s-1 cm-2
|
background-subtracted flux inferred from the modified
elliptical aperture for each science energy band
|
| photflux_aper90_hilim |
double[6] |
photons s-1 cm-2
|
upper limit on the confidence interval of the
"photflux_aper90" value for each science energy band
|
| photflux_aper90_lolim |
double[6] |
photons s-1 cm-2
|
lower limit on the confidence interval of the
"photflux_aper90" value for each science energy band
|
| flux_aper |
double[6] |
ergs s-1 cm-2
|
background-subtracted flux inferred from the modified source region for each science energy band
|
| flux_aper_hilim |
double[6] |
ergs s-1 cm-2
|
upper limit on the confidence interval of the "flux_aper"
value for each science energy band
|
| flux_aper_lolim |
double[6] |
ergs s-1 cm-2
|
lower limit on the confidence interval of the "flux_aper"
value for each science energy band
|
| flux_aper90 |
double[6] |
ergs s-1 cm-2
|
background-subtracted flux inferred from the modified
elliptical aperture for each science energy band
|
| flux_aper90_hilim |
double[6] |
ergs s-1 cm-2
|
upper limit on the confidence interval of the "flux_aper90"
value for each science energy band
|
| flux_aper90_lolim |
double[6] |
ergs s-1 cm-2
|
lower limit on the confidence interval of the "flux_aper90"
value for each science energy band
|
| flux_powlaw_aper |
double[6] |
ergs s-1 cm-2
|
power law model energy flux inferred from the modified source region for each science energy band
|
| flux_powlaw_aper_hilim |
double[6] |
ergs s-1 cm-2
|
upper limit on the confidence interval of the "flux_powlaw_aper"
value for each science energy band
|
| flux_powlaw_aper_lolim |
double[6] |
ergs s-1 cm-2
|
lower limit on the confidence interval of the "flux_powlaw_aper"
value for each science energy band
|
| flux_powlaw_aper90 |
double[6] |
ergs s-1 cm-2
|
power law model energy flux inferred from the modified
elliptical aperture for each science energy band
|
| flux_powlaw_aper90_hilim |
double[6] |
ergs s-1 cm-2
|
upper limit on the confidence interval of the "flux_powlaw_aper90"
value for each science energy band
|
| flux_powlaw_aper90_lolim |
double[6] |
ergs s-1 cm-2
|
lower limit on the confidence interval of the "flux_powlaw_aper90"
value for each science energy band
|
| flux_bb_aper |
double[6] |
ergs s-1 cm-2
|
black body model energy flux inferred from the modified
source region for each science energy band
|
| flux_bb_aper_hilim |
double[6] |
ergs s-1 cm-2
|
upper limit on the confidence interval of the "flux_bb_aper"
value for each science energy band
|
| flux_bb_aper_lolim |
double[6] |
ergs s-1 cm-2
|
lower limit on the confidence interval of the "flux_bb_aper"
value for each science energy band
|
| flux_bb_aper90 |
double[6] |
ergs s-1 cm-2
|
black body model energy flux inferred from the modified
elliptical aperture for each science energy band
|
| flux_bb_aper90_hilim |
double[6] |
ergs s-1 cm-2
|
upper limit on the confidence interval of the "flux_bb_aper90"
value for each science energy band
|
| flux_bb_aper90_lolim |
double[6] |
ergs s-1 cm-2
|
lower limit on the confidence interval of the "flux_bb_aper90"
value for each science energy band
|
| psf_frac_aper |
double[6] |
|
fraction of the PSF included in the modified source region for each science energy band
|
| psf_frac_aperbkg |
double[6] |
|
fraction of the PSF included in the modified background region for each science energy band
|
| psf_frac_aper90 |
double[6] |
|
fraction of the PSF included in the modified elliptical aperture
for each science energy band
|
| psf_frac_aper90bkg |
double[6] |
|
fraction of the PSF included in the modified elliptical
background aperture for each science energy band
|
|
|
Spectral Properties
|
alpha |
double |
|
best-fit power law photon index (γ, defined as
FE ∼ E-γ)
|
| alpha_hilim |
double |
|
upper limit on the confidence interval of the "alpha"
value
|
| alpha_lolim |
double |
|
lower limit on the confidence interval of the "alpha"
value
|
| flux_powlaw |
double |
ergs s-1 cm-2
|
integrated 0.5-7.0 keV flux derived from the best-fitting
power law spectral fit
|
| flux_powlaw_hilim |
double |
ergs s-1 cm-2
|
upper limit on the confidence interval of the "flux_powlaw"
value
|
| flux_powlaw_lolim |
double |
ergs s-1 cm-2
|
lower limit on the confidence interval of the "flux_powlaw"
value
|
| nh_powlaw |
double |
N HI atoms 1020 cm-2
|
best-fit power law NH value
|
| nh_powlaw_hilim |
double |
N HI atoms 1020 cm-2
|
upper limit on the confidence interval of the "nh_powlaw"
value
|
| nh_powlaw_lolim |
double |
N HI atoms 1020 cm-2
|
lower limit on the confidence interval of the "nh_powlaw"
value
|
| powlaw_stat |
double |
|
χ2 (data variance) statistic per degree of
freedom for the best-fitting power law spectral fit
|
| kt |
double |
keV |
best-fit thermal (black body) temperature (kT)
|
| kt_hilim |
double |
keV |
upper limit on the confidence interval of the "kt"
value
|
| kt_lolim |
double |
keV |
lower limit on the confidence interval of the "kt"
value
|
| flux_bb |
double |
ergs s-1 cm-2
|
best-fit thermal (black body) spectral fit flux
|
| flux_bb_hilim |
double |
ergs s-1 cm-2
|
upper limit on the confidence interval of the "flux_bb"
value
|
| flux_bb_lolim |
double |
ergs s-1 cm-2
|
lower limit on the confidence interval of the "flux_bb"
value
|
| nh_bb |
double |
|
best-fit thermal (black body) NH value
|
| nh_bb_hilim |
double |
|
upper limit on the confidence interval of the "nh_bb"
value
|
| nh_bb_lolim |
double |
|
lower limit on the confidence interval of the "nh_bb"
value
|
| bb_stat |
double |
|
χ2 (data variance) statistic per degree of
freedom for the best-fitting thermal (black body) spectral
fit
|
| hard_<x><y> |
double[3] |
|
hardness ratio
for a pair of ACIS science energy bands, where ''<x>''
and ''<y>'' represent the higher (harder) and lower
(softer) energy band designations, respectively.
|
| hard_<x><y>_hilim |
double[3] |
|
upper confidence limit on
''hard_<x><y>'' value
|
| hard_<x><y>_lolim |
double[3] |
|
lower confidence limit on
''hard_<x><y>'' value
|
|
|
Source Variability
|
ks_prob |
double[6] |
|
Kolmogorov-Smirnov test probability for each science energy band
|
| kp_prob |
double[6] |
|
Kuiper's test probability for each science energy band
|
| var_prob |
double[6] |
|
Gregory-Loredo variability probability for each science energy band
|
| var_index |
integer[6] |
|
variability index in the range [0,10] for each science energy band that combines the
var_prob value with the fractions of the multi-resolution
light curve output by the Gregory-Loredo analysis that are
within 3 σ and 5 σ of the average count rate, to
evaluate whether the source region flux is uniform
throughout the observation
|
| var_mean |
double[6] |
counts s-1
|
time-averaged value of the source region count rate for each science energy band
|
| var_sigma |
double[6] |
counts s-1
|
time-averaged 1 σ statistical variability of the source region count rate for each science energy band
|
| var_min |
double[6] |
counts s-1
|
minimum value of the source region count rate for each science energy band
|
| var_max |
double[6] |
counts s-1
|
maximum value of the source region count rate for each science energy band
|
| dither_warning_flag |
boolean |
|
TRUE if the highest statistically significant peak in the
power spectrum of the source region count rate for each science energy band
occurs either at the
dither frequency of the
observation or at a beat frequency of the
dither frequency.
Otherwise, the value is FALSE.
|
|
|
Source Timing Information
|
livetime |
double |
s |
effective exposure time for the observation after applying
the good time intervals
and deadtime correction factor
|
|
|
Source Instrument Information
|
detector |
string |
|
detector elements over which the background region bounding box
dithers
during the observation: HRC-I, HRC-S, or ACIS-<n>,
where <n> is string of the CCD Ids (e.g. "ACIS-78");
see the ACIS focal
plane figure in the POG.
|
|
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