ACIS
ACIS DOSE Registered-Photon-Map
The steps we took to compute the dose map are;
- Level 1 Event files for a specified month are obtained from archive.
- Image data including I2, I3, S2, S3 CCDs are extracted from all event files.
- All the extracted image data were merged to create a month long exposure map for the month.
- The exposure map is opened with ds9, and check a distribution of count rates against energy. From this, estimate the upper threshold value. Any events beyond this upper threshold are assumed erroneous events such as bad pixels.
- Using this upper threshold, the data is filtered, and create a cleaned exposure map for the month.
- The exposure map from each month from the Sep 1999 is added up to create a cumulative exposure map for each month.
- Using fimgstatistic, we compute count rate statistics for each CCDs.
- For observations with high data drop rates (e.g., Crab nebula, Cas A), we corrected the observations by adding events.
Please check more detail plots at Telemetered Photon Dose Trend page.
Statistics: # IMAGE NPIX MEAN RMS MIN MAX ACIS_nov17 6004901 9.495 34.859 0.0 7149 I2 node 0 262654 7.352981 3.324236 0.0 54.0 I2 node 1 262654 7.580980 14.627800 0.0 7149.0 I2 node 2 262654 7.394592 3.267046 0.0 83.0 I2 node 3 262654 7.494541 19.266064 0.0 7048.0 I3 node 0 262654 8.438865 4.582687 0.0 1336.0 I3 node 1 262654 8.257144 18.368639 0.0 6320.0 I3 node 2 262654 7.913933 3.338799 0.0 86.0 I3 node 3 262654 8.013014 3.496563 0.0 138.0 S2 node 0 262654 11.856867 26.598577 0.0 1107.0 S2 node 1 262654 12.868873 25.189814 0.0 1164.0 S2 node 2 262654 14.633628 50.052591 0.0 2093.0 S2 node 3 262654 15.684564 51.882505 0.0 2195.0 S3 node 0 262654 19.149927 31.339484 0.0 1793.0 S3 node 1 262654 20.577046 53.496692 0.0 3601.0 S3 node 2 262654 20.504553 75.006338 0.0 3378.0 S3 node 3 262654 18.179898 75.994314 0.0 3474.0
Statistics: IMAGE NPIX MEAN RMS MIN MAX ACIS_total 6004901 2158.580 2802.229 0.0 121753 I2 node 0 262654 1852.255630 363.172633 383.0 10342.0 I2 node 1 262654 1949.946130 504.692819 404.0 70300.0 I2 node 2 262654 7.394592 3.267046 0.0 83.0 I2 node 3 262654 1987.249449 512.284259 390.0 28420.0 I3 node 0 262654 2101.341907 519.507057 384.0 8225.0 I3 node 1 262654 2184.182562 1635.298227 395.0 51371.0 I3 node 2 262654 1917.366632 352.753222 374.0 10662.0 I3 node 3 262654 8.013014 3.496563 0.0 138.0 S2 node 0 262654 2511.385432 390.443548 1441.0 21644.0 S2 node 1 262654 12.868873 25.189814 0.0 1164.0 S2 node 2 262654 2954.326850 608.540332 2029.0 27574.0 S2 node 3 262654 2900.683802 461.709348 1776.0 51700.0 S3 node 0 262654 4477.908866 2028.254479 1963.0 25198.0 S3 node 1 262654 5672.097973 2203.945133 0.0 28199.0 S3 node 2 262654 4446.239752 1204.800209 1845.0 24657.0 S3 node 3 262654 3425.703416 640.615802 2108.0 24335.0
Aug 2017 | May 2017 | Feb 2017 | Nov 2016 |
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The Mean Detrended CTI
We report CTIs with a refined data definition. CTIs were computed for the temperature dependency corrected data. Please see CTI page for detailed explanation. CTI's are computed for Mn K alpha, and defined as slope/intercept x10^4 of row # vs ADU. Data file: here
Imaging CCDs
Spectral CCDs
Backside CCDs
Focal Plane Temperature
Nov 2017 Focal Temperature
The Mean (max) FPT: | |
---|---|
-113.85 | +/- 2.69 C |
Mean Width: | |
0.79 | +/- 0.28 days |
Averaged Focal Plane Temperature
We are using 10 period moving averages to show trends of peak temperatures and peak widths. Note, the gaps in the width plot are due to missing/corrupted data.
Focal Plane Temperature, Sun Angle and Altitude
Bad Pixels
The plots below were generated with a new warm pixel finding script. Please see Acis Bad Pixel Page for details.
Front Side CCDs
Back Side CCD (CCD5)
Science Instrument Background Rates
Name | Low (keV) | High(KeV) | Description |
---|---|---|---|
SSoft | 0.00 | 0.50 | Super soft photons |
Soft | 0.50 | 1.00 | Soft photons |
Med | 1.00 | 3.00 | Moderate energy photons |
Hard | 3.00 | 5.00 | Hard Photons |
Harder | 5.00 | 10.00 | Very Hard photons |
Hardest | 10.00 | Beyond 10 keV |
The following three plots show trends of SIB from year 2000. CCDs shown here are CCD3, CCD5, and CCD7. Fitted lines are linear fit after eliminating extreme outliers. For >10 keV plots, 2 lines are fit. One is with a 13 keV filter, and another without.
CCD 3
CCD 5
CCD 7
ACIS Histogram Mode Trends
We collected data from acis histogram mode data, and created trend plots of peak portions and peak widths against time (DOM). The peaks were estimated by fitting a simple Gaussian on three peaks (Al, Ti, and Mn), and the widths were estimated by a width at the half max from the peak.
All histogram data are taken under TIMED and GRADED_HIST mode, SIM position is at an external calibration source position, the focal temperature is around -119.7 C, and parameter settings in aciselec, acistemp are set to about same for all.
CCD 3, Peak Position
CCD 3, Peak Widths
CCD 3, Count Rates
HRC
DOSE of Central 4K Pore-Pairs
Please refer to Maximum Dose Trends for more details.
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_11_2017.fits 16777216 0.036 0.192 0.000 8.000
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_08_1999_11_2017.fits 16777216 5.083 5.280 0.000 293.000
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_11_2017.fits 16777216 0.019 0.203 0.000 25.000
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_08_1999_11_2017.fits 16777216 16.679 29.853 0.000 1715.000
Max dose trend plots corrected for events that "pile-up"
in the center of the taps due to bad position information.
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Aug 2017 | May 2017 | Feb 2017 | Nov 2016 |
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Aug 2017 | May 2017 | Feb 2017 | Nov 2016 |
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Gratings
Focus
We plot the width of the zero order streak of ACIS/HETG observations and the width of the zero order image for HRC/LETG observations of point sources. No significant defocusing trend is seen at this time. See Gratings Focus pages.
PCAD
ACA Trending
Gyro Bias Drift
Radiation History
Radiation Zone Timing
Plotted below are radiation zone timing plots based on the following definitions of radiation zone:
- RADZONE - Ephin levels (in any of the E1300,P4GM,P41GM channels) are more than 1/3 of RADMON safing thresholds.
- RADMON - Radmon is disabled for radiation zone (as commanded based on OFLS model, for comparison with actual radiation levels).
- PERIGEE - Time of closest earth approach (for comparison)
Radiation Count Rates of Nov 2017
Sun Spot History
Trending
Quarterly Trends
- HRMA Heater
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
OHRTHR03 | 295.24 | 1.102e-03 | 3.355e-03 | 3.940e-02 | K | RT 5: HRMA FORWARD APERTURE PLATE |
OHRTHR09 | 294.72 | 0.10 | 4.532e-01 | 2.484e+00 | K | RT 105: HRMA CAP |
OHRTHR17 | 294.59 | 0.11 | 4.758e-01 | 2.453e+00 | K | RT 125: HSA OUTER CYNLINDER |
OHRTHR24 | 294.90 | 0.19 | 6.087e-01 | 2.654e-02 | K | RT 12: HRMA AFT HEATER PLATE |
OHRTHR38 | 296.29 | 0.97 | 2.110e+00 | 6.203e+00 | K | RT 120: HRMA AFT COLLIMATOR OUTER CYLINDER |
OHRTHR52 | 294.58 | 0.11 | 4.756e-01 | 2.688e+00 | K | RT 100: HRMA CAP |
- HRMA Thermal
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
4RT568T | 295.29 | 1.16 | 8.337e+00 | -2.964e+01 | K | RT 568 - HRMA TEMP |
4RT569T | 294.87 | 0.24 | 1.950e+00 | 1.445e+01 | K | RT 569 - HRMA TEMP |
4RT570T | 294.70 | 0.14 | 1.099e+00 | 3.044e+00 | K | RT 570 - HRMA TEMP |
4RT575T | 299.18 | 1.62 | 1.107e+01 | -7.105e+01 | K | RT 575 - OB CONE TEMP |
4RT576T | 291.28 | 1.21 | 8.541e+00 | -6.291e+01 | K | RT 576 - OB CONE TEMP |
4RT578T | 297.71 | 2.20 | 1.096e+01 | -5.077e+01 | K | RT 578 - OB CONE TEMP |
- MUPS
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
PM1THV1T | 331.85 | 8.13 | 7.987e+00 | -7.932e+02 | K | MUPS 1 THRUSTER VALVE 01 TEMP |
PLINE02T | 320.68 | 9.61 | -1.517e+00 | 5.416e+02 | K | PROP LINE TEMP 02 |
PLINE03T | 318.18 | 11.95 | 4.329e-01 | 6.675e+02 | K | PROP LINE TEMP 03 |
PLINE04T | 304.38 | 11.62 | 8.152e+00 | 6.499e+02 | K | PROP LINE TEMP 04 |
Envelope Trending
Spacecraft Motions
TSC and FA Cummulative Moter Distance
HETG and LETG Cummulative Insertion Counts
HETG/LETG Insertion/Retraction Angle
Reaction Wheel Rotations
Links to Past Monthly Reports
Year | Month | |||||||||||
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2017 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | ||
2016 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2015 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2014 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2013 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2012 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2011 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2010 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2009 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2008 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2007 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2006 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2005 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2004 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2003 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2002 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2001 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2000 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
1999 | Jul | Aug | Sep | Oct | Nov | Dec |