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 | 39002 | 38998 | 36186 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1337845 ccd2:28729 ccd3:38446 ccd4:28391 ccd5:36288 ccd7:27715 |
filter=Medium date-obs=2008-05-20T14:05:09 object=V2491 Cyg roll_angle=54.7059326172 |
|
mos2 | 39005 | 39004 | 36131 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1310424 ccd2:26135 ccd3:28212 ccd4:22675 ccd5:24676 ccd6:36168 ccd7:27719 |
filter=Medium date-obs=2008-05-20T14:05:08 object=V2491 Cyg roll_angle=54.7059326172 |
25 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 Mar 15 20:59:05 2012
This data set was last accessed on Thu Mar 15 20:59:05 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0552270501
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