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 | 45116 | 45116 | 45114 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:65358 ccd2:40067 ccd3:54630 ccd4:47674 ccd5:41273 ccd7:38508 |
filter=CalClosed date-obs=2009-11-16T21:10:23 object=Mkn 421 roll_angle=119.354057312 |
|
pn | 8169 | 8169 | 8169 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:13550 ccd2:3622 ccd3:2591 ccd4:1398052 ccd5:14819 ccd6:4307 ccd7:75732 ccd8:12830 ccd9:4126 ccd10:6586 ccd11:2988 ccd12:2590 |
filter=Thick date-obs=2009-11-16T18:07:10 object=Mkn 421 timedel=0.05 roll_angle=119.354057312 |
48 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 Tue Jun 5 09:55:04 2012
This data set was last accessed on Tue Jun 5 09:55:04 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0411083201
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