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 | 5166 | 5166 | 5166 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1553 ccd2:800 ccd3:979 ccd4:868 ccd5:796 ccd6:907 ccd7:768 |
filter=Thin1 date-obs=2003-09-15T19:05:28 object=SAX J0635+0521 roll_angle=88.5140228271 |
|
mos2 | 5169 | 5169 | 5168 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1478 ccd2:772 ccd3:863 ccd4:703 ccd5:762 ccd6:996 ccd7:754 |
filter=Thin1 date-obs=2003-09-15T19:05:28 object=SAX J0635+0521 roll_angle=88.5140228271 |
8 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 = 6.13
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 Thu Jun 27 19:51:11 2013
This data set was last accessed on Thu Jun 27 19:51:11 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0146870201
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