ACIS E0102-72 Calibration Observations
An oxygen rich supernova remnant, E0102 is observed every 6 months at various chip positions to monitor low energy response.
Analysis: We use a PERL script to call CIAO dm (data model) tools which return background subtracted counts in several energy bands. Input is the observation level 2 events file (evt2). dmlist is called several times to gather header information for bookkeeping, aimpoint, and target location, with dmcoords used to convert between coordinate systems. Several source regions are pre-defined based on off-axis distance. These range from a circle of radius 50 pixels (for sources less than 400 pixels off-axis) to a 100 X 130 pixel ellipse (sources greater than 1200 pixels off-axis). Source regions are written in sky coordinates. Appropriate background regions are the same size and shape as the source region are selected by referring to the source chip coordinates so that the background remains on-chip and streak-free. An IDL-generated plot is included as a link in each observation row to inspect the regions selected. Finally, dmextract is called with several energy filters and the source and background regions parameters. Net counts are read from the output FITS table and reported on the following pages.
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CTI Corrected:
I3 S3 Other Chips
CTI Uncorrected:
I3 S3 Other Chips