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 |
---|---|---|---|---|---|---|---|---|---|
mos2 | 25025 | 25004 | 24619 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:29615 ccd2:4607 ccd3:4952 ccd4:4508 ccd5:4555 ccd6:5693 ccd7:4717 |
filter=Medium date-obs=2003-04-26T21:05:16 object=Markarian 6 roll_angle=253.097183228 |
|
pn | 4523 | 4523 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:16566 ccd2:16751 ccd3:10197 ccd4:18495 ccd5:16089 ccd6:15991 ccd7:15468 ccd8:18833 ccd9:13065 ccd10:10418 ccd11:8128 ccd12:4636 |
filter=CalClosed date-obs=2003-04-26T12:34:40 object=Markarian 6 timedel=0.19 roll_angle=253.097183228 |
25 source(s) in memory Iteration: 1 Images: |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 = 6.13
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 Tue Jun 4 00:38:06 2013
This data set was last accessed on Tue Jun 4 00:38:06 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0144230101
Position of field target = 6 52 12.32 74 25 36.8
Current telescope = xmm
Current detector = all
Processing mode = proc
Processing status = Warning, bgd. level not computed because source mask doesn't exist
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