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 |
---|---|---|---|---|---|---|---|---|---|
mos2 | 4849 | 4477 | 3141 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:17740 ccd2:9083 ccd3:10289 ccd4:8343 ccd5:9118 ccd6:11768 ccd7:9852 |
filter=Medium date-obs=2003-06-23T09:04:05 object=IRAS20126+4104 roll_angle=30.232793808 |
|
pn | 0 | 1.00 | 1.00 | 0/0 | Yes | orig clean |
date-obs=2003-06-23T11:04:43 object= roll_angle=30.232793808 |
1 source(s) in memory Iteration: 2 Images: |mos2 |pn |
|
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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 Fri Feb 24 08:49:11 2012
This data set was last accessed on Fri Feb 24 08:49:11 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0135970401
Position of field target = 20 14 26.00 41 13 32.0
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