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 | 9998 | 9998 | 9996 | 1.00 | 4.35 | 0.004/0.004/0.004 | Yes | orig clean | ccd1:47249 ccd2:1950 ccd3:2568 ccd4:2999 ccd5:2393 ccd7:2124 |
filter=Thick date-obs=2009-01-05T06:25:18 object=AB Dor roll_angle=202.304519653 |
|
pn | 10000 | 10000 | 9998 | 1.00 | 4.35 | 0.12/0.12/0.12 | Yes | orig clean | ccd4:145342 |
filter=Thick date-obs=2009-01-05T06:28:06 object=AB Dor timedel=0.00 roll_angle=202.304519653 |
6 source(s) in memory Iteration: 2 Images: |mos1 |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 Sat Nov 26 22:08:06 2011
This data set was last accessed on Sat Nov 26 22:08:06 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0412580401
Position of field target = 5 28 44.83 -65 26 54.9
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