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 | 53714 | 52231 | 38458 | 1.00 | 4.35 | 0.014/0.013/0.003 | Yes | orig clean | ccd1:342177 ccd2:50928 ccd3:63991 ccd4:50132 ccd5:54644 ccd6:61361 ccd7:49259 |
filter=Medium date-obs=2001-10-09T21:47:36 object=ESO 141-G55 roll_angle=251.323364258 |
|
mos2 | 53763 | 52630 | 38894 | 1.00 | 4.35 | 0.014/0.012/0.0027 | Yes | orig clean | ccd1:341605 ccd2:52083 ccd3:56950 ccd4:45377 ccd5:49901 ccd6:64175 ccd7:54174 |
filter=Medium date-obs=2001-10-09T21:48:01 object=ESO 141-G55 roll_angle=251.323364258 |
29 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 Sat Dec 24 01:51:06 2011
This data set was last accessed on Sat Dec 24 01:51:06 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0101040501
Position of field target = 19 21 14.20 -58 40 12.8
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