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 | 5889 | 4568 | 3718 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:41387 ccd2:23067 ccd3:28270 ccd4:22718 ccd5:24420 ccd6:26551 ccd7:21925 |
filter=Thin1 date-obs=2003-09-21T10:11:30 object=SAX J0635+0521 roll_angle=90.3751220703 |
|
mos2 | 5983 | 4698 | 3724 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:45913 ccd2:24699 ccd3:23008 ccd4:22123 ccd5:20921 ccd6:31737 ccd7:26441 |
filter=Thin1 date-obs=2003-09-21T10:11:30 object=SAX J0635+0521 roll_angle=90.3751220703 |
3 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 Aug 10 18:37:07 2012
This data set was last accessed on Fri Aug 10 18:37:07 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0146870401
Position of field target = 6 35 18.00 5 33 11.0
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