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 | 30545 | 29713 | 23709 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:77864 ccd2:43200 ccd3:52477 ccd4:44657 ccd5:45424 ccd7:39745 |
filter=Medium date-obs=2012-08-16T03:26:36 object=LMC survey 33 roll_angle=61.3858680725 |
|
pn | 22887 | 16693 | 12812 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:185930 ccd2:180843 ccd3:123005 ccd4:198250 ccd5:158926 ccd6:119646 ccd7:164751 ccd8:164590 ccd9:111269 ccd10:115424 ccd11:115178 ccd12:88168 |
filter=Thin1 date-obs=2012-08-16T03:48:50 object=LMC survey 33 timedel=0.07 roll_angle=61.3858680725 |
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 Mon May 6 00:38:03 2013
This data set was last accessed on Mon May 6 00:38:03 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0690743301
Position of field target = 5 24 10.38 -68 50 54.3
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