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 | 36554 | 36443 | 25747 | 1.00 | 4.35 | 0.034/0.034/0.016 | Yes | orig clean | ccd1:808334 ccd2:60903 ccd3:77546 ccd4:63197 ccd5:70369 ccd6:78913 ccd7:61693 |
filter=Medium date-obs=2002-09-26T05:38:18 object=LMC X-1 roll_angle=97.3578414917 |
|
mos2 | 36598 | 36582 | 25704 | 1.00 | 4.35 | 0.029/0.028/0.013 | Yes | orig clean | ccd1:774196 ccd2:60550 ccd3:65569 ccd4:49400 ccd5:56278 ccd6:80859 ccd7:64586 |
filter=Medium date-obs=2002-09-26T05:38:18 object=LMC X-1 roll_angle=97.3578414917 |
56 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 Fri Jan 6 09:55:05 2012
This data set was last accessed on Fri Jan 6 09:55:05 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0023940401
Position of field target = 5 39 38.00 -69 44 36.0
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