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 | 23223 | 16081 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:2270293 ccd2:26371 ccd3:51310 ccd4:38452 ccd5:34268 ccd6:52495 ccd7:28487 |
filter=Thick date-obs=2002-09-25T09:33:55 object=U1728-16 roll_angle=271.622314453 |
|
mos2 | 23139 | 17704 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:2369223 ccd2:35518 ccd3:46219 ccd4:32142 ccd5:32560 ccd6:52058 ccd7:40717 |
filter=Thick date-obs=2002-09-25T09:33:55 object=U1728-16 roll_angle=271.622314453 |
79 source(s) in memory Iteration: 1 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 Fri May 3 00:58:02 2013
This data set was last accessed on Fri May 3 00:58:02 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0090340601
Position of field target = 17 31 44.17 -16 57 41.6
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = Warning, bgd. level not computed because source mask doesn't exist
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