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 | 13401 | 13401 | 13400 | 1.00 | 4.35 | 0.0027/0.0027/0.0027 | Yes | orig clean | ccd2:2784 ccd3:3645 ccd4:2916 ccd5:2945 ccd6:3372 ccd7:2535 |
filter=Thin1 date-obs=2004-05-16T01:32:26 object=RX J0513.9-6951 roll_angle=336.320648193 |
|
mos2 | 13406 | 13406 | 13405 | 1.00 | 4.35 | 0.0027/0.0027/0.0027 | Yes | orig clean | ccd2:2795 ccd3:3044 ccd4:2606 ccd5:2982 ccd6:3709 ccd7:3159 |
filter=Thin1 date-obs=2004-05-16T01:32:25 object=RX J0513.9-6951 roll_angle=336.320648193 |
17 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 27 09:55:07 2011
This data set was last accessed on Tue Dec 27 09:55:07 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0151412501
Position of field target = 5 13 50.80 -69 51 47.0
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