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 | 15101 | 15101 | 12544 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:17809 ccd3:21961 ccd4:17502 ccd5:18291 ccd6:20759 ccd7:17019 |
filter=Thin1 date-obs=2003-09-05T08:11:16 object=BY Cam roll_angle=111.332420349 |
|
mos2 | 15106 | 15106 | 12480 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:17966 ccd3:19682 ccd4:15786 ccd5:17530 ccd6:22485 ccd7:18945 |
filter=Thin1 date-obs=2003-09-05T08:11:15 object=BY Cam roll_angle=111.332420349 |
7 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 Mon May 21 03:54:14 2012
This data set was last accessed on Mon May 21 03:54:14 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0148590801
Position of field target = 5 42 48.90 60 51 31.8
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