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 | 57970 | 57962 | 57959 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:168854 ccd2:7337 ccd3:8948 ccd4:8799 ccd5:7395 ccd7:7258 |
filter=Thick date-obs=2012-09-18T18:08:44 object=Capella roll_angle=83.7744674683 |
|
pn | 12501 | 12501 | 12501 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:532565 |
filter=Thick date-obs=2012-09-18T18:13:48 object=Capella timedel=0.00 roll_angle=83.7744674683 |
6 source(s) in memory Iteration: 2 Images: |mos1 |pn |
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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 00:38:02 2013
This data set was last accessed on Fri May 3 00:38:02 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0510781101
Position of field target = 5 16 41.36 45 59 53.0
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