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 | 14402 | 14402 | 12225 | 1.00 | 4.35 | 0.019/0.019/0.013 | Yes | orig clean | ccd2:19803 ccd3:26859 ccd4:21111 ccd5:23021 ccd6:26219 ccd7:19288 |
filter=Medium date-obs=2004-06-22T09:56:56 object=Cyg X-3 roll_angle=34.4305229187 |
|
mos2 | 14680 | 14680 | 13336 | 1.00 | 4.35 | 0.035/0.035/0.03 | Yes | orig clean | ccd1:412412 ccd2:20277 ccd3:23106 ccd4:18410 ccd5:19573 ccd6:27565 ccd7:21931 |
filter=Medium date-obs=2004-06-22T09:56:46 object=Cyg X-3 roll_angle=34.4305229187 |
21 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 Sun Dec 18 21:47:24 2011
This data set was last accessed on Sun Dec 18 21:47:24 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0165360201
Position of field target = 20 32 26.20 40 57 20.7
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