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 | 37596 | 37596 | 37595 | 1.00 | 4.35 | 0.029/0.029/0.029 | Yes | orig clean | ccd1:1927507 ccd2:21901 ccd3:37442 ccd4:27643 ccd5:28129 ccd7:23030 |
filter=Medium date-obs=2010-03-09T13:52:27 object=4U 1702-429 roll_angle=95.6190414429 |
|
mos2 | 37600 | 37600 | 37600 | 1.00 | 4.35 | 0.0089/0.0089/0.0089 | Yes | orig clean | ccd1:1839794 ccd2:25418 ccd3:31272 ccd4:23534 ccd5:24628 ccd6:36756 ccd7:27901 |
filter=Medium date-obs=2010-03-09T13:52:27 object=4U 1702-429 roll_angle=95.6190414429 |
9 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 Fri Jan 6 08:15:10 2012
This data set was last accessed on Fri Jan 6 08:15:10 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0604030101
Position of field target = 17 6 15.31 -43 2 8.6
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