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 |
---|---|---|---|---|---|---|---|---|---|
pn | 712 | 552 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:1755 ccd2:1983 ccd3:2382 ccd4:1982 ccd5:1551 ccd6:2035 ccd7:1493 ccd8:1548 ccd9:2086 ccd10:1388 ccd11:1459 ccd12:1994 |
filter=Medium date-obs=2002-04-19T23:57:20 object=Finger/Draco 1 timedel=0.19 roll_angle=47.7118911743 |
0 source(s) in memory Iteration: 1 Images: |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 May 2 16:24:50 2013
This data set was last accessed on Thu May 2 16:24:50 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0110660901
Position of field target = 17 0 0.00 59 40 0.0
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = Production of fullrun_pn_xmm0110660901_pi300-10000_totbgd.evt failed
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