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 | 26806 | 26635 | 26507 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:21737 ccd3:31613 ccd4:26774 ccd5:24332 ccd7:21538 |
filter=Thin1 date-obs=2008-05-07T01:34:55 object=Mrk 421 roll_angle=303.526824951 |
|
mos2 | 26458 | 26219 | 26026 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:22700 ccd3:25253 ccd4:20895 ccd5:24130 ccd6:28383 ccd7:22969 |
filter=Thin1 date-obs=2008-05-07T01:34:55 object=Mrk 421 roll_angle=303.526824951 |
40 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
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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 Thu Apr 5 20:24:58 2012
This data set was last accessed on Thu Apr 5 20:24:58 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0502030101
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