Instrument Team Monitoring of ACIS
ACIS Monitoring
Radiation Damage Monitoring
Charge transfer inefficiency (CTI) and particle background
Trailing pixel - lost charge re-emitted into a trailing pixel
Instrument Monitoring
Corner pixel distribution
Overclock levels
Focal plane temperature
Calibration Monitoring
Detector gain
Spectral line centroid and width - Gaussian fits at 5.9 and 1.5 keV
Contamination
Detection efficiency - measuring changes at high energy from CTI
Related Pages
Bev LaMarr's images of recent raw frames
ACIS CTI background detrending (major update 11/12/10)
Preliminary analysis of Oct 2003 CTI change (now understood as sacrificial charge from the particle background)
Alternating exposure mode data analysis (was used for removing the FI CCD CTI background dependence, now superceded)
Global change history:
- April 2007 - Temperature filters all updated to better reflect the temperature dependence of each monitored quantity. In most cases, the new temperature filters also increase the total amount of usable data. CTI monitoring is unchanged and uses all available data and applies a temperature-dependent correction. Trailing pixel and spectral line monitoring have the temperature upper limit raised from -119.7 to -119.4. Detector gain and detection efficiency monitoring have the temperature upper limit raised from -119.7 to -119.0. Corner pixel monitoring used to use all available data and now has a temperature upper limit of -119.0.
- September 2008 - Added focal plane temperature page.
- April 2012 - Added overclock levels page.
- Jan 2013 - Completely overhauled line fits.
- Jan 2013 - Switched postscript links to PDF
Last updated March 23, 2023
Web page by Catherine E. Grant (
cgrant@mit.edu )
MIT Kavli Institute for Astrophysics and Space Research
Massachusetts Institute of Technology
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