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 | 29341 | 29341 | 29341 | 1.00 | 4.35 | 0.003/0.003/0.003 | Yes | orig clean | ccd2:6883 ccd3:8748 ccd4:6600 ccd5:7660 ccd6:8018 ccd7:6472 |
filter=Medium date-obs=2001-02-15T19:50:24 object=UX Arietis roll_angle=241.775772095 |
|
mos2 | 29348 | 29348 | 29348 | 1.00 | 4.35 | 0.0038/0.0038/0.0038 | Yes | orig clean | ccd1:227872 ccd2:6600 ccd3:7786 ccd4:6260 ccd5:6914 ccd6:8850 ccd7:6842 |
filter=Medium date-obs=2001-02-15T19:39:56 object=UX Arietis roll_angle=241.775772095 |
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 = 6.11
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 Wed Nov 30 17:05:03 2011
This data set was last accessed on Wed Nov 30 17:05:03 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111390301
Position of field target = 3 26 35.39 28 42 54.3
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