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 | 32997 | 32597 | 25685 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:62846 ccd2:24546 ccd3:30306 ccd4:24263 ccd5:25552 ccd6:29779 ccd7:23621 |
filter=Thin1 date-obs=2002-01-09T22:57:39 object=1RXSJ160518.8+32490 roll_angle=135.647583008 |
|
mos2 | 32984 | 32600 | 25880 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:65632 ccd2:23410 ccd3:26898 ccd4:20593 ccd5:25303 ccd6:30750 ccd7:24728 |
filter=Thin1 date-obs=2002-01-09T22:57:38 object=1RXSJ160518.8+32490 roll_angle=135.647583008 |
23 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 Wed Jul 25 18:19:06 2012
This data set was last accessed on Wed Jul 25 18:19:06 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0073140301
Position of field target = 16 5 18.80 32 49 7.0
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