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 | 39472 | 39469 | 39469 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:40097 ccd2:8721 ccd3:10614 ccd4:8499 ccd5:9074 ccd6:10035 ccd7:8631 |
filter=Thick date-obs=2002-02-09T16:19:33 object=kappa1 Ceti roll_angle=255.441757202 |
|
mos2 | 39203 | 39203 | 29829 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:35504 ccd3:40106 ccd4:32499 ccd5:34670 ccd6:44343 ccd7:38247 |
filter=Medium date-obs=2002-02-09T16:19:27 object=kappa1 Ceti roll_angle=255.441757202 |
7 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 Tue Jun 11 14:16:27 2013
This data set was last accessed on Tue Jun 11 14:16:27 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111410101
Position of field target = 3 19 21.70 3 22 12.7
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