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 | 32589 | 32558 | 32556 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:311932 ccd2:9761 ccd3:12638 ccd4:10031 ccd5:10103 ccd7:9995 |
filter=Thick date-obs=2006-09-22T22:10:51 object=IGR J17497-2821 roll_angle=271.206451416 |
|
mos2 | 32326 | 32324 | 32323 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:11093 ccd3:11759 ccd4:9379 ccd5:13652 ccd6:13338 ccd7:11506 |
filter=Thick date-obs=2006-09-22T22:10:55 object=IGR J17497-2821 roll_angle=271.206451416 |
19 source(s) in memory Iteration: 2 Images: |mos1 |mos2 |
|
|
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 Mon Jul 9 16:56:08 2012
This data set was last accessed on Mon Jul 9 16:56:08 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0410580401
Position of field target = 17 49 37.80 -28 21 18.0
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