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 | 7366 | 7363 | 6275 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:10603 ccd2:5695 ccd3:7019 ccd4:5602 ccd5:6150 ccd6:6642 ccd7:5499 |
filter=Thin1 date-obs=2003-10-08T07:48:04 object=SAX J0635+0521 roll_angle=95.1610794067 |
|
mos2 | 7371 | 7371 | 6539 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:10455 ccd2:5534 ccd3:5826 ccd4:4931 ccd5:5411 ccd6:7121 ccd7:5631 |
filter=Thin1 date-obs=2003-10-08T07:48:03 object=SAX J0635+0521 roll_angle=95.1610794067 |
6 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 Tue May 29 09:55:03 2012
This data set was last accessed on Tue May 29 09:55:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0146871101
Position of field target = 6 35 18.00 5 33 11.0
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