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 | 21401 | 21401 | 21401 | 1.00 | 4.35 | 0.018/0.018/0.018 | Yes | orig clean | ccd2:23439 ccd3:45522 ccd4:34132 ccd5:34716 ccd6:44068 ccd7:24928 |
filter=Thick date-obs=2004-03-26T14:36:19 object=Serpens X-1 roll_angle=87.551902771 |
|
mos2 | 21406 | 21406 | 21406 | 1.00 | 4.35 | 0.018/0.018/0.018 | Yes | orig clean | ccd2:29521 ccd3:39942 ccd4:25954 ccd5:30863 ccd6:45819 ccd7:35160 |
filter=Thick date-obs=2004-03-26T14:36:19 object=Serpens X-1 roll_angle=87.551902771 |
70 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 Sat Dec 17 22:08:03 2011
This data set was last accessed on Sat Dec 17 22:08:03 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0084020601
Position of field target = 18 39 57.00 5 2 6.0
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