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 | 13421 | 5221 | 5221 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1026860 ccd2:54754 ccd3:103654 ccd4:66318 ccd5:69468 ccd6:96347 ccd7:56730 |
filter=Medium date-obs=2003-10-17T01:04:50 object=GRS 1915+05 roll_angle=260.22366333 |
|
mos2 | 13427 | 5107 | 5107 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1045087 ccd2:69272 ccd3:94197 ccd4:68488 ccd5:62752 ccd6:99388 ccd7:74286 |
filter=Medium date-obs=2003-10-17T01:04:50 object=GRS 1915+05 roll_angle=260.22366333 |
97 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 Mon May 20 00:42:04 2013
This data set was last accessed on Mon May 20 00:42:04 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0112990501
Position of field target = 19 15 11.00 10 56 44.0
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