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 |
---|---|---|---|---|---|---|---|---|---|
mos2 | 3294 | 3294 | 3294 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:48244 ccd2:23661 ccd3:37008 ccd4:22520 ccd5:38698 ccd6:41695 ccd7:23013 |
filter=CalClosed date-obs=2003-09-25T01:43:36 object=G32.45+0.1 roll_angle=268.961608887 |
|
pn | 0 | 1.00 | 1.00 | 0/0 | Yes | orig clean |
date-obs=2003-09-25T03:21:37 object= roll_angle=268.961608887 |
10 source(s) in memory Iteration: 2 Images: |mos2 |pn |
|
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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 Jul 13 09:55:04 2012
This data set was last accessed on Fri Jul 13 09:55:04 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0136030101
Position of field target = 18 50 6.70 -0 25 40.0
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