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 | 48753 | 46252 | 29671 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:142760 ccd2:79902 ccd3:99491 ccd4:78805 ccd5:82610 ccd6:92912 ccd7:81552 |
filter=Medium date-obs=2004-04-10T08:05:35 object=PSR J0737-3039 roll_angle=274.312164307 |
|
mos2 | 49060 | 47441 | 33258 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:4773 ccd2:83590 ccd3:84961 ccd4:69012 ccd5:80242 ccd6:98248 ccd7:83598 |
filter=Medium date-obs=2004-04-10T08:05:44 object=PSR J0737-3039 roll_angle=274.312164307 |
31 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 29 09:55:05 2012
This data set was last accessed on Thu Mar 29 09:55:05 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0164560301
Position of field target = 7 37 51.25 -30 39 40.7
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