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 | 10176 | 10176 | 10176 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:397368 ccd2:2312 ccd3:3400 ccd4:2654 ccd5:2635 ccd7:2323 |
filter=Thick date-obs=2010-11-14T20:45:17 object=Mkn 421 roll_angle=116.346794128 |
|
pn | 8237 | 8235 | 8235 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:6215 ccd2:2338 ccd3:1862 ccd4:836397 ccd5:7006 ccd6:2584 ccd7:34755 ccd8:6313 ccd9:2551 ccd10:3259 ccd11:2032 ccd12:1990 |
filter=Thick date-obs=2010-11-14T21:13:35 object=Mkn 421 timedel=0.05 roll_angle=116.346794128 |
19 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 Sat Apr 7 09:59:03 2012
This data set was last accessed on Sat Apr 7 09:59:03 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0656381301
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