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 | 10899 | 10899 | 10899 | 1.00 | 4.35 | 0.087/0.087/0.087 | Yes | orig clean | ccd2:62497 ccd3:132394 ccd4:85562 ccd5:87977 ccd6:135355 ccd7:70744 |
filter=Thick date-obs=2003-10-06T06:52:55 object=Crab roll_angle=87.9064941406 |
|
mos2 | 11165 | 6745 | 6733 | 1.00 | 4.35 | 0.09/0.054/0.054 | Yes | orig clean | ccd1:785229 ccd2:96629 ccd3:121231 ccd4:85489 ccd5:80385 ccd6:120909 ccd7:99223 |
filter=Thick date-obs=2003-10-06T06:52:55 object=Crab roll_angle=87.9064941406 |
169 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 12:10:31 2011
This data set was last accessed on Fri Dec 16 12:10:31 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0160960301
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