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 | 7168 | 7166 | 6795 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:40496 ccd3:85478 ccd4:65295 ccd5:51871 ccd6:68171 ccd7:45154 |
filter=Thick date-obs=2002-03-07T15:33:01 object=Crab roll_angle=267.339111328 |
|
mos2 | 7192 | 7189 | 7189 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:56932 ccd3:73110 ccd4:53136 ccd5:62215 ccd6:86322 ccd7:64507 |
filter=Thick date-obs=2002-03-07T15:33:06 object=Crab roll_angle=267.339111328 |
177 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 Thu May 17 15:43:05 2012
This data set was last accessed on Thu May 17 15:43:05 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0153750201
Position of field target = 5 34 32.00 22 0 52.0
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