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 | 5749 | 5749 | 5749 | 1.00 | 4.35 | 0.084/0.084/0.084 | Yes | orig clean | ccd2:31669 ccd3:72741 ccd4:51191 ccd5:45438 ccd7:35387 |
filter=Thick date-obs=2007-03-05T07:23:52 object=Crab roll_angle=267.260162354 |
|
mos2 | 5754 | 5754 | 5754 | 1.00 | 4.35 | 0.089/0.089/0.089 | Yes | orig clean | ccd2:43337 ccd3:56530 ccd4:41489 ccd5:48416 ccd6:66340 ccd7:48403 |
filter=Thick date-obs=2007-03-05T07:23:52 object=Crab roll_angle=267.260162354 |
162 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 Sat Nov 26 22:08:07 2011
This data set was last accessed on Sat Nov 26 22:08:07 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0412590601
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