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 | 11612 | 11573 | 5377 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:31504 ccd2:16177 ccd3:20437 ccd4:15863 ccd5:16280 ccd6:24497 ccd7:15853 |
filter=Medium date-obs=2001-07-11T05:55:42 object=PSR 1259-63/SS2883 roll_angle=286.638671875 |
|
mos2 | 11594 | 11594 | 5404 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:31028 ccd2:15409 ccd3:17479 ccd4:13799 ccd5:15283 ccd6:19571 ccd7:21916 |
filter=Medium date-obs=2001-07-11T05:55:42 object=PSR 1259-63/SS2883 roll_angle=286.638671875 |
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 = 6.11
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 Tue Mar 6 01:21:02 2012
This data set was last accessed on Tue Mar 6 01:21:02 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0092820201
Position of field target = 13 2 47.68 -63 50 8.6
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