Detector | Exposure (Original/High-E Flare Cleaned/Low-E Cleaned) | Image binning | Plate scale ("/pixel) | Bgd. level (orig/High-E flare cleaned/cleaned, counts/sq. arcmin/s) | GTI file | Bgd. light curves | Roll angle | CCD counts | Extra info |
---|---|---|---|---|---|---|---|---|---|
mos1 | 12093 | 10813 | 9931 | 1.00 | 4.35 | 0.016/0.0055/0.002 | Yes | orig clean | ccd2:15162 ccd3:18409 ccd4:14661 ccd5:14902 ccd6:17121 ccd7:14401 |
filter=Medium date-obs=2001-03-04T22:30:16 object=Her X-1 roll_angle=96.2734069824 |
|
mos2 | 12943 | 11087 | 9872 | 1.00 | 4.35 | 0.021/0.0069/0.0027 | Yes | orig clean | ccd1:82975 ccd2:19729 ccd3:22190 ccd4:17572 ccd5:19288 ccd6:24845 ccd7:21339 |
filter=Medium date-obs=2001-03-04T22:20:40 object=Her X-1 roll_angle=96.2734069824 |
13 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
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Python version = 2.5.4 (r254:67916, Aug 14 2009, 18:07:15) [GCC 4.1.1 20070105 (Red Hat 4.1.1-52)]
Headas version = 6.11
XAssist version = 1.000
SAS version = xmmsas_20110223_1801-11.0.0
numpy version = 1.3.0
Pyfits version = 2.1.1
XAssist originally started on this data set at Tue Dec 27 22:08:09 2011
This data set was last accessed on Tue Dec 27 22:08:09 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111060101
Position of field target = 16 57 49.80 35 20 32.6
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = OK
Detection method = eboxdetect
Batch processing enabled
Place data, logs, etc. in field subdirectories
Image analysis will be over range of allowed energies
Will analyze each ccd separately
Log files: processing messages |error messages |all messages (very detailed) |source logs