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 | 7956 | 7956 | 7955 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:4203 ccd2:2407 ccd3:2802 ccd4:2292 ccd5:2685 ccd7:2366 |
filter=Thin1 date-obs=2011-05-20T16:45:24 object=LMC X-3 offset roll_angle=322.739257812 |
|
mos2 | 7959 | 7959 | 7958 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:3730 ccd2:2061 ccd3:2294 ccd4:1873 ccd5:1844 ccd6:2584 ccd7:1899 |
filter=Thin1 date-obs=2011-05-20T16:45:23 object=LMC X-3 offset roll_angle=322.739257812 |
15 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 Sun Jun 2 23:18:03 2013
This data set was last accessed on Sun Jun 2 23:18:03 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0671420201
Position of field target = 5 45 0.00 -63 30 0.0
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