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 | 10182 | 10177 | 10177 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:490175 ccd2:2550 ccd3:4039 ccd4:3024 ccd5:3419 ccd7:2558 |
filter=Thick date-obs=2010-11-12T20:51:58 object=Mkn 421 roll_angle=116.343406677 |
|
pn | 8237 | 8237 | 8237 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:7687 ccd2:2571 ccd3:1999 ccd4:979433 ccd5:8459 ccd6:2910 ccd7:43745 ccd8:7873 ccd9:2824 ccd10:4005 ccd11:2225 ccd12:2174 |
filter=Thick date-obs=2010-11-12T21:20:16 object=Mkn 421 timedel=0.05 roll_angle=116.343406677 |
17 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 Mar 30 02:19:49 2012
This data set was last accessed on Fri Mar 30 02:19:49 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0656380801
Position of field target = 11 4 27.31 38 12 31.8
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