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 | 22302 | 22302 | 22301 | 1.00 | 4.35 | 0.0051/0.0051/0.0051 | Yes | orig clean | ccd1:222093 ccd2:4642 ccd3:5869 ccd4:6295 ccd5:5659 ccd7:4671 |
filter=Thick date-obs=2010-08-20T01:16:26 object=gamma Cassiopeiae roll_angle=43.8490715027 |
|
mos2 | 22300 | 22300 | 22299 | 1.00 | 4.35 | 0.004/0.004/0.004 | Yes | orig clean | ccd1:223667 ccd2:4794 ccd3:5348 ccd4:4332 ccd5:4500 ccd6:5688 ccd7:4963 |
filter=Thick date-obs=2010-08-20T01:16:34 object=gamma Cassiopeiae roll_angle=43.8490715027 |
|
pn | 22351 | 22351 | 22350 | 1.00 | 4.35 | 0.19/0.19/0.19 | Yes | orig clean | ccd4:561499 |
filter=Thick date-obs=2010-08-20T01:18:30 object=gamma Cassiopeiae timedel=0.00 roll_angle=43.8490715027 |
6 source(s) in memory Iteration: 2 Images: |mos1 |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 Thu Nov 24 22:08:03 2011
This data set was last accessed on Thu Nov 24 22:08:03 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0651670501
Position of field target = 0 56 42.53 60 43 0.3
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