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 | 1713 | 1713 | 1713 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:9542 ccd3:21879 ccd4:15370 ccd5:14459 ccd7:10799 |
filter=Thick date-obs=2007-03-04T17:52:02 object=Crab roll_angle=267.26171875 |
|
mos2 | 1355 | 1355 | 1355 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:10352 ccd3:13505 ccd4:9793 ccd5:11288 ccd6:15703 ccd7:11669 |
filter=Thick date-obs=2007-03-04T17:57:58 object=Crab roll_angle=267.26171875 |
39 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 Mon Mar 19 09:55:02 2012
This data set was last accessed on Mon Mar 19 09:55:02 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0412590501
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