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 | 43587 | 43582 | 43518 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:50219 ccd2:14494 ccd3:17185 ccd4:15556 ccd5:17867 ccd7:13943 |
filter=Medium date-obs=2012-03-31T01:50:02 object=IGR J17494-3030 roll_angle=92.6883850098 |
|
mos2 | 43595 | 43595 | 43594 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:50991 ccd2:13598 ccd3:15201 ccd4:11262 ccd5:12001 ccd6:20886 ccd7:13407 |
filter=Medium date-obs=2012-03-31T01:50:01 object=IGR J17494-3030 roll_angle=92.6883850098 |
48 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 = 6.13
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 Sat May 4 22:28:00 2013
This data set was last accessed on Sat May 4 22:28:00 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0694040201
Position of field target = 17 49 23.70 -30 29 59.0
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