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 | 49266 | 49266 | 40974 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:170305 ccd2:52033 ccd3:74548 ccd4:63027 ccd5:50083 ccd6:64048 ccd7:49712 |
filter=CalClosed date-obs=2001-09-10T23:36:45 object=47 Cassiopeiae roll_angle=42.6273002625 |
|
pn | 40175 | 40175 | 40174 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:324172 |
filter=Medium date-obs=2001-09-11T02:21:19 object=47 Cassiopeiae timedel=0.00 roll_angle=42.6273002625 |
23 source(s) in memory Iteration: 2 Images: |mos1 |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 = 6.13
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 Jun 6 00:38:03 2013
This data set was last accessed on Thu Jun 6 00:38:03 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111520101
Position of field target = 2 5 7.42 77 16 52.8
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