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 | 13462 | 12349 | 8144 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:5104 ccd2:39819 ccd3:53533 ccd4:40707 ccd5:39321 ccd7:36969 |
filter=Thin1 date-obs=2010-02-22T20:26:17 object=IGR J16393-4643 roll_angle=93.9218521118 |
|
mos2 | 13489 | 12413 | 8210 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:4718 ccd2:34227 ccd3:39910 ccd4:30224 ccd5:35309 ccd6:43501 ccd7:38571 |
filter=Thin1 date-obs=2010-02-22T20:26:17 object=IGR J16393-4643 roll_angle=93.9218521118 |
|
pn | 19253 | 14262 | 11054 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:313286 |
filter=Thin1 date-obs=2010-02-22T20:31:26 object=IGR J16393-4643 timedel=0.00 roll_angle=93.9218521118 |
8 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |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 Thu Apr 5 16:24:52 2012
This data set was last accessed on Thu Apr 5 16:24:52 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0604520201
Position of field target = 16 39 5.40 -46 42 12.0
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