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_oct18 6004901 7.889 12.182 0.0 725 I2 node 0 262654 12.336687 4.704146 0.0 100.0 I2 node 1 262654 12.358125 4.754106 0.0 116.0 I2 node 2 262654 12.204207 4.572138 0.0 106.0 I2 node 3 262654 12.178645 4.705448 0.0 52.0 I3 node 0 262654 12.753992 5.006077 0.0 119.0 I3 node 1 262654 11.534736 5.233986 0.0 137.0 I3 node 2 262654 10.945334 4.086627 0.0 90.0 I3 node 3 262654 12.036895 4.757816 0.0 209.0 S2 node 0 262654 5.045121 2.602746 0.0 155.0 S2 node 1 262654 5.028377 2.692319 0.0 49.0 S2 node 2 262654 5.127386 2.832523 0.0 375.0 S2 node 3 262654 5.162831 2.746564 0.0 326.0 S3 node 0 262654 11.653263 3.946536 0.0 60.0 S3 node 1 262654 13.222627 4.915794 0.0 183.0 S3 node 2 262654 13.020784 4.153915 0.0 81.0 S3 node 3 262654 11.876159 3.910204 0.0 36.0
Statistics: IMAGE NPIX MEAN RMS MIN MAX ACIS_total 6004901 2244.368 2905.188 0.0 125999 I2 node 0 262654 1938.831523 383.996198 412.0 11012.0 I2 node 1 262654 2040.276625 535.448204 429.0 84055.0 I2 node 2 262654 2071.073477 438.949729 428.0 10901.0 I2 node 3 262654 2076.508822 536.703762 417.0 28504.0 I3 node 0 262654 2198.574725 543.851188 406.0 8739.0 I3 node 1 262654 2280.321390 1675.074651 429.0 55043.0 I3 node 2 262654 2007.927958 372.162392 408.0 11354.0 I3 node 3 262654 1998.606088 400.231959 360.0 31496.0 S2 node 0 262654 2609.251214 408.481007 1480.0 21800.0 S2 node 1 262654 2767.399020 617.645392 1622.0 15224.0 S2 node 2 262654 3061.615637 627.981801 2069.0 27713.0 S2 node 3 262654 3011.588989 480.105396 1826.0 55691.0 S3 node 0 262654 4632.443114 2091.659669 2040.0 27048.0 S3 node 1 262654 5855.404606 2235.806678 0.0 28883.0 S3 node 2 262654 4619.033169 1231.387276 1968.0 25030.0 S3 node 3 262654 3564.257863 650.192720 2187.0 24597.0
Jul 2018 | Apr 2018 | Jan 2018 | Oct 2017 |
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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
Oct 2018 Focal Temperature
The Mean (max) FPT: | |
---|---|
-111.59 | +/- 4.34 C |
Mean Width: | |
2.38 | +/- 2.53 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_10_2018.fits 16777216 0.115 0.736 0.000 66.000
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_08_1999_10_2018.fits 16777216 5.563 5.697 0.000 302.000
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_10_2018.fits 16777216 0.051 0.239 0.000 5.000
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_08_1999_10_2018.fits 16777216 17.776 32.504 0.000 1730.000
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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Jul 2018 | Apr 2018 | Jan 2018 | Oct 2017 |
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Jul 2018 | Apr 2018 | Jan 2018 | Oct 2017 |
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Gratings
Grating Trends/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 Trends pages.
Gratings Resolving Power
We plot E/dE vs. E for fits to detected lines with fwhm_error/fwhm less than 0.15 for the plus and minus arms of HEG, MEG, and LEG. Also shown are conservative (dotted line) and optimistic (dashed line) pre-launch resolving power expectations.
We have selected only calibration observations of Capella, HR1099, and Sigma Gem. See MIT technotes for a parallel analysis.
Year 2014 - | |
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Letg minus side | Letg plus side |
Metg minus side | Metg plus side |
Hetg minus side | Hetg plus side |
PCAD
ACA Trending
Gyro Bias Drift
Radiation History
Radiation Count Rates of Oct 2018
Sun Spot History
SIM
SIM Shift and Twist
SIM Shift and Twist Trend The following plots show trends of SIM shifts (dy and dz) and twist (dtheta). All quantities are directly taken from pcaf*_asol1.fits files. The units are mm for dy and dz, and degree for dtheta. We fit three lines separated before and after (Days of Mission)= 1400 (May 21, 2003), 2700 (Dec 11, 2006), and 4400 (Aug 07, 2011). The unit of slopes are mm per day or degree per day.
The sudden shift around DOM = 1400, 2700 and 4400 are due to fid light drift (see a memo by Aldcroft fiducial light drift). On the dtheta plot, two tracks are clearly observed. The track around 0.01 is due to HRC-I, and all others are clustered around -0.002. For more detail, please see SIM Shift and Twist Trend page
Trending
Quarterly Trends
- EPS Batteries
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
eb2ci | 0.304 | 0.110 | (-1.91+/-0.10)e-5 | -0.002+/-0.000 | AMP | BATT 2 CHARGE CURRENT |
---|---|---|---|---|---|---|
eb2di | 0.025 | 0.234 | (0.00+/-0.00)e0 | (-1.58+/-0.14)e-4 | AMP | BATT 2 DISCHARGE CURRENT |
eb2v | 32.337 | 0.129 | (-1.86+/-0.07)e-4 | 0.010+/-0.001 | V | BATT 2 VOLTAGE |
ecnv1v | 14.892 | 0.006 | (4.32+/-0.34)e-6 | (-7.12+/-0.43)e-4 | V | CONV 1 +15V OUTPUT |
ecnv2v | 14.843 | 0.010 | (5.78+/-1.22)e-6 | -0.003+/-0.000 | V | CONV 2 +15V OUTPUT |
ecnv3v | 15.290 | 0.004 | (-4.27+/-0.38)e-6 | (4.02+/-0.13)e-4 | V | CONV 3 +15V OUTPUT |
- Spacecraft Electronics
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
elbi | 55.174 | 1.296 | (4.73+/-1.70)e-4 | 0.064+/-0.008 | AMP | LOAD BUS CURRENT |
---|---|---|---|---|---|---|
elbv | 28.686 | 0.196 | (4.78+/-0.25)e-4 | -0.033+/-0.001 | V | LOAD BUS VOLTAGE |
- OBA Heater
Previous Quarter | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
oobthr04 | 298.409 | 1.517 | 0.002+/-0.000 | 0.018+/-0.062 | K | RT 27: HRMA STRUT |
---|---|---|---|---|---|---|
oobthr12 | 296.673 | 2.094 | 0.003+/-0.000 | -0.055+/-0.075 | K | RT 35: OBA FWD CONE |
oobthr26 | 300.071 | 3.070 | 0.004+/-0.000 | -0.632+/-0.089 | K | RT 48: OBA AFT CONE |
oobthr38 | 283.187 | 0.362 | (1.78+/-0.11)e-5 | 0.003+/-0.001 | K | RT 60: TFTE FWD CYLINDER |
oobthr44 | 298.617 | 2.099 | 0.004+/-0.000 | 0.062+/-0.074 | K | RT 66: TFTE AFT CYLINDER |
oobthr50 | 293.408 | 1.827 | 0.002+/-0.000 | -0.270+/-0.074 | K | RT 76: S/C STRUT |
Spacecraft Motions
TSC and FA Cummulative Moter Distance
HETG and LETG Cummulative Insertion Counts
HETG/LETG Insertion/Retraction Angle
Reaction Wheel Rotations