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 | 31939 | 31931 | 31929 | 1.00 | 4.35 | 0.0063/0.0063/0.0063 | Yes | orig clean | ccd2:12954 ccd3:22834 ccd4:16298 ccd5:17310 ccd6:22477 ccd7:13950 |
filter=Thick date-obs=2001-02-18T17:39:17 object=1700-37 roll_angle=92.313911438 |
|
mos2 | 32552 | 32548 | 32548 | 1.00 | 4.35 | 0.016/0.016/0.016 | Yes | orig clean | ccd1:1329212 ccd2:16649 ccd3:20787 ccd4:15400 ccd5:15699 ccd6:23482 ccd7:19270 |
filter=Thick date-obs=2001-02-18T17:29:50 object=1700-37 roll_angle=92.313911438 |
39 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 Tue Dec 20 22:08:10 2011
This data set was last accessed on Tue Dec 20 22:08:10 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0083280201
Position of field target = 17 3 56.80 -37 50 39.1
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