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 | 14365 | 14360 | 14040 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:18220 ccd3:26059 ccd4:19451 ccd5:21488 ccd6:24832 ccd7:17738 |
filter=Medium date-obs=2004-06-20T10:02:51 object=Cyg X-3 roll_angle=36.1687049866 |
|
pn | 4621 | 4621 | 4621 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:13806 ccd2:13886 ccd3:8616 ccd4:15290 ccd5:13109 ccd6:13347 ccd7:12946 ccd8:15918 ccd9:10870 ccd10:8614 ccd11:7014 ccd12:4141 |
filter=CalClosed date-obs=2004-06-20T08:20:07 object=Cyg X-3 timedel=0.07 roll_angle=36.1687049866 |
8 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 = 6.11
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 Sat May 26 09:55:03 2012
This data set was last accessed on Sat May 26 09:55:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0165360101
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