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 | 23661 | 23405 | 21168 | 1.00 | 4.35 | 0.016/0.014/0.0096 | Yes | orig clean | ccd1:703825 ccd2:20547 ccd3:27642 ccd4:21216 ccd5:21100 ccd7:20611 |
filter=Medium date-obs=2006-02-26T17:10:04 object=RS Oph roll_angle=96.6331863403 |
|
mos2 | 23405 | 23085 | 20467 | 1.00 | 4.35 | 0.014/0.012/0.0064 | Yes | orig clean | ccd2:26579 ccd3:29361 ccd4:23483 ccd5:25420 ccd6:33962 ccd7:27785 |
filter=Thin1 date-obs=2006-02-26T17:10:00 object=RS Oph roll_angle=96.6331863403 |
6 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 Fri Nov 25 14:49:16 2011
This data set was last accessed on Fri Nov 25 14:49:16 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0410180101
Position of field target = 17 50 13.20 -6 42 28.0
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