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 | 20652 | 20642 | 19617 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:28116 ccd2:16447 ccd3:22293 ccd4:17701 ccd5:16784 ccd7:15777 |
filter=Medium date-obs=2011-08-29T07:02:51 object=IRAS 05020-2941 roll_angle=61.7343673706 |
|
pn | 8028 | 6268 | 2896 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:38839 ccd2:37734 ccd3:25655 ccd4:40798 ccd5:32097 ccd6:24293 ccd7:41148 ccd8:37422 ccd9:25390 ccd10:30756 ccd11:30572 ccd12:23213 |
filter=Medium date-obs=2011-08-29T07:25:12 object=IRAS 05020-2941 timedel=0.07 roll_angle=61.7343673706 |
8 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 = 6.13
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 Jun 2 07:10:05 2013
This data set was last accessed on Sun Jun 2 07:10:05 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0672900501
Position of field target = 5 4 0.70 -29 36 54.8
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