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 | 9851 | 5107 | 5093 | 1.00 | 4.35 | 0.087/0.044/0.044 | Yes | orig clean | ccd1:596279 ccd2:53729 ccd3:123309 ccd4:87650 ccd5:77130 ccd6:113127 ccd7:60093 |
filter=Thick date-obs=2002-03-08T19:51:30 object=Crab roll_angle=267.336853027 |
|
mos2 | 11505 | 11435 | 11435 | 1.00 | 4.35 | 0.089/0.087/0.087 | Yes | orig clean | ccd2:86644 ccd3:113834 ccd4:80816 ccd5:97877 ccd6:133814 ccd7:99738 |
filter=Thick date-obs=2002-03-08T19:18:41 object=Crab roll_angle=267.336853027 |
185 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 Wed Dec 28 13:57:06 2011
This data set was last accessed on Wed Dec 28 13:57:06 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0153750501
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