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 | 5249 | 5249 | 5249 | 1.00 | 4.35 | 0.087/0.087/0.087 | Yes | orig clean | ccd2:28956 ccd3:65515 ccd4:47644 ccd5:46044 ccd7:32878 |
filter=Thick date-obs=2009-02-24T12:02:48 object=Crab roll_angle=276.725830078 |
|
mos2 | 5255 | 5255 | 5255 | 1.00 | 4.35 | 0.089/0.089/0.089 | Yes | orig clean | ccd2:39453 ccd3:50751 ccd4:36283 ccd5:43926 ccd6:60775 ccd7:44714 |
filter=Thick date-obs=2009-02-24T12:02:48 object=Crab roll_angle=276.725830078 |
144 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 Dec 16 12:58:14 2011
This data set was last accessed on Fri Dec 16 12:58:14 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0412592501
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