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 | 31139 | 30691 | 26049 | 1.00 | 4.35 | 0.026/0.024/0.016 | Yes | orig clean | ccd1:284298 ccd2:56924 ccd3:71617 ccd4:58804 ccd5:61113 ccd7:53657 |
filter=Thin1 date-obs=2008-05-30T08:22:19 object=V2491 Cyg roll_angle=46.4118270874 |
|
mos2 | 31137 | 30797 | 25916 | 1.00 | 4.35 | 0.021/0.02/0.012 | Yes | orig clean | ccd1:276678 ccd2:48216 ccd3:52462 ccd4:42911 ccd5:48234 ccd6:66134 ccd7:50795 |
filter=Thin1 date-obs=2008-05-30T08:22:20 object=V2491 Cyg roll_angle=46.4118270874 |
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 Thu Dec 22 17:59:21 2011
This data set was last accessed on Thu Dec 22 17:59:21 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0552270601
Position of field target = 19 43 2.10 32 19 12.8
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