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 | 24003 | 22979 | 21137 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:60894 ccd2:18367 ccd3:22607 ccd4:18662 ccd5:19255 ccd6:21275 ccd7:18220 |
filter=Thick date-obs=2003-05-30T11:07:25 object=zeta Puppis roll_angle=310.790130615 |
|
pn | 21851 | 21851 | 21849 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:172600 |
filter=Medium date-obs=2003-05-30T23:38:30 object=zeta Puppis timedel=0.00 roll_angle=310.790130615 |
5 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 Fri Sep 7 08:52:03 2012
This data set was last accessed on Fri Sep 7 08:52:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0159360101
Position of field target = 8 3 35.05 -40 0 11.3
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