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 | 11711 | 11711 | 11326 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:179071 ccd2:4550 ccd3:5873 ccd4:4462 ccd5:4954 ccd7:4424 |
filter=Thick date-obs=2011-11-28T23:29:27 object=Mkn 421 roll_angle=116.346588135 |
|
pn | 10534 | 10534 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:7425 ccd2:7794 ccd3:5153 ccd4:8261 ccd5:7257 ccd6:6787 ccd7:6950 ccd8:8533 ccd9:6067 ccd10:5303 ccd11:5072 ccd12:3673 |
filter=CalClosed date-obs=2011-11-29T03:50:00 object=Mkn 421 timedel=0.07 roll_angle=116.346588135 |
4 source(s) in memory Iteration: 1 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 = 6.13
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 Sun Aug 11 05:10:03 2013
This data set was last accessed on Sun Aug 11 05:10:03 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0658800801
Position of field target = 11 4 27.31 38 12 31.8
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