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 | 28039 | 28015 | 25199 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:153462 ccd2:20820 ccd3:27962 ccd4:20431 ccd5:25714 ccd6:550304 ccd7:31131 |
filter=Medium date-obs=2001-09-03T10:13:10 object=1E 1613-5055 off roll_angle=270.707244873 |
|
mos2 | 28036 | 28002 | 25250 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:160991 ccd2:430166 ccd3:25714 ccd4:18722 ccd5:20216 ccd6:27306 ccd7:202970 |
filter=Medium date-obs=2001-09-03T10:13:09 object=1E 1613-5055 off roll_angle=270.707244873 |
131 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 Sep 1 13:39:06 2012
This data set was last accessed on Sat Sep 1 13:39:06 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0113050701
Position of field target = 16 17 30.00 -50 55 5.0
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