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 | 17600 | 17600 | 17599 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:3429 ccd3:4670 ccd4:4964 ccd5:3940 ccd6:4581 ccd7:3336 |
filter=Thin1 date-obs=2004-05-26T05:45:40 object=RX J0513.9-6951 roll_angle=2.4695930481 |
|
mos2 | 17605 | 17605 | 17604 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:3830 ccd3:3791 ccd4:3369 ccd5:4576 ccd6:5112 ccd7:3963 |
filter=Thin1 date-obs=2004-05-26T05:45:41 object=RX J0513.9-6951 roll_angle=2.4695930481 |
20 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 Thu May 9 13:20:05 2013
This data set was last accessed on Thu May 9 13:20:05 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0151412701
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