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_feb15 6004901 8.186 13.033 0.0 1861 I2 node 0 262654 7.185688 3.188100 0.0 62.0 I2 node 1 262654 7.480994 3.561504 0.0 502.0 I2 node 2 262654 7.360120 3.223152 0.0 63.0 I2 node 3 262654 7.352103 5.576301 0.0 1513.0 I3 node 0 262654 7.828798 3.650450 0.0 55.0 I3 node 1 262654 8.078702 7.929561 0.0 1861.0 I3 node 2 262654 7.296066 3.187932 0.0 81.0 I3 node 3 262654 7.315676 3.248323 0.0 91.0 S2 node 0 262654 9.725245 6.843284 0.0 98.0 S2 node 1 262654 10.286026 6.005104 0.0 87.0 S2 node 2 262654 14.007525 10.478198 0.0 1270.0 S2 node 3 262654 16.881576 11.255541 0.0 409.0 S3 node 0 262654 13.379515 13.996296 0.0 351.0 S3 node 1 262654 15.839115 13.504099 0.0 244.0 S3 node 2 262654 18.785769 19.692259 0.0 283.0 S3 node 3 262654 15.906540 25.098970 0.0 343.0
Statistics: IMAGE NPIX MEAN RMS MIN MAX ACIS_total 6004901 1864.979 2445.779 0.0 108038 I2 node 0 262654 1566.331275 299.935269 293.0 9086.0 I2 node 1 262654 1651.172091 413.906427 326.0 38041.0 I2 node 2 262654 1681.196440 351.551578 326.0 9207.0 I2 node 3 262654 1679.114159 422.970066 310.0 28020.0 I3 node 0 262654 1764.342361 420.170842 308.0 6924.0 I3 node 1 262654 1851.806140 1402.453051 313.0 35468.0 I3 node 2 262654 1618.484150 290.527392 299.0 8312.0 I3 node 3 262654 1604.195454 311.086065 284.0 27230.0 S2 node 0 262654 2183.872855 316.843158 1155.0 21225.0 S2 node 1 262654 2323.565671 508.059917 1217.0 12860.0 S2 node 2 262654 2562.227562 485.020076 1540.0 19358.0 S2 node 3 262654 2487.315999 345.879403 1447.0 42378.0 S3 node 0 262654 3881.613940 1797.793241 1595.0 13564.0 S3 node 1 262654 5054.983680 2079.934231 0.0 14039.0 S3 node 2 262654 3860.056392 985.810965 1584.0 9377.0 S3 node 3 262654 2995.327708 452.030222 1713.0 10356.0
Nov 2014 | Aug 2014 | May 2014 | Feb 2014 |
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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
Feb 2015 Focal Temperature
The Mean (max) FPT: | |
---|---|
-114.45 | +/- 2.73 C |
Mean Width: | |
1.15 | +/- 0.76 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 |
HRC
DOSE of Central 4K Pore-Pairs
Please refer to Maximum Dose Trends for more details.
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_02_2015.fits 16777216 0.005 0.0674 0.0 2.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_08_1999_02_2015.fits 16777216 4.309 4.896 0.0 292.0
No Data
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_08_1999_02_2015.fits 16777216 15.588 27.267 0.0 1681.0
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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Feb 2015 | Aug 2014 | May 2014 | Feb 2014 |
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Nov 2014 | Aug 2014 | May 2014 | Feb 2014 |
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HRMA Focus
Plots below show various characteristics of detected imaging sources. Standard level 2 data products (*src2.fits) are used. Only observations with focus (sim_x) within 0.01 mm of nominal value for given SI configuration are used. Sources are also filtered for strength (SNR > 15).
For individual detectors, please go to MTA SRC2 Monitoring page.
Source Sky Position
PSF vs Time
Source Ellipse Roundness
80% Encircled Energy Radius
Signal-to-Noise Ratio
Rotation
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
ACIS-S and HRC Celestial Location Monitoring
Science Instrument Positional Change Monitoring
The following plots are the difference between coordinates obtained from Chandra observations and those obtained from existing catalogs vs time in day of mission.
The following steps are taken to generate these plots.
- all observations with grating are selected
- even if the observation is not grating one, if it is a known point source, it is added to the list.
- observed ra, jan, target ra, jan, nominal ra, jan and a ratio of a target elliptical to psf (psfratio are extracted from src fits files.
- the observations with psfratio smaller than 4 are selected
- the differences between observed coordinates and targeted coordinates (if not available nominal coordinates) are computed
- if the differences are larger than 6 arcsec, the points are dropped
The large dispersion around DOM ~ 2400 (Jan 2005) are all due to none grating Capella observations. Many observations are off-axis observations (e.g., obsid 6558).
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 Feb 2015
Sun Spot History
Trending
Quarterly Trends
- OBA Heaters
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
OOBTHR04 | 294.97 | 0.90 | 1.648e+00 | -2.071e+01 | K | RT 27: HRMA STRUT |
OOBTHR08 | 292.48 | 3.10 | 1.391e+01 | 6.307e+02 | K | RT 31: OBA CONE |
OOBTHR14 | 290.41 | 2.45 | 1.107e+01 | 4.831e+02 | K | RT 37: OBA CONE |
OOBTHR22 | 291.35 | 2.95 | 1.180e+01 | 5.358e+02 | K | RT 44: OBA CONE |
OOBTHR40 | 288.46 | 1.77 | 8.437e+00 | 3.534e+02 | K | RT 62: TFTE CONE |
OOBTHR59 | 295.56 | 1.39 | 1.778e+00 | -2.152e+01 | K | RT 152: OBA CONE |
- HRMA Heaters
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
OHRTHR02 | 295.30 | 2.917e-03 | -9.632e-03 | 6.374e-02 | K | RT 2: HRMA FORWARD APERTURE PLATE |
OHRTHR19 | 294.58 | 1.332e-02 | 2.353e-02 | 5.781e-02 | K | RT 132: HRMA AFT HEATER PLATE |
OHRTHR44 | 295.29 | 7.815e-03 | -3.082e-02 | -1.025e-02 | K | RT 1: HRMA FORWARD APERTURE PLATE |
OHRTHR59 | 295.30 | 4.270e-03 | -2.700e-03 | 6.340e-02 | K | RT 119: HRMA PRECOLLIMATOR PLATE 10 |
Envelope Trending
PCAD Temperature
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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2015 | Jan | |||||||||||
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 |