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 | 22238 | 18883 | 10947 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:555032 ccd2:102783 ccd3:125102 ccd4:105577 ccd5:101865 ccd6:126586 ccd7:104335 |
filter=Medium date-obs=2000-05-23T13:05:20 object=N132D roll_angle=339.771057129 |
|
mos2 | 22325 | 19160 | 10403 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:553224 ccd2:107006 ccd3:123811 ccd4:96987 ccd5:109894 ccd6:137636 ccd7:117627 |
filter=Medium date-obs=2000-05-23T13:05:19 object=N132D roll_angle=339.771057129 |
8 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 23 00:38:03 2013
This data set was last accessed on Thu May 23 00:38:03 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0125100301
Position of field target = 5 25 8.00 -69 38 24.0
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