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 | 55270 | 55257 | 52249 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:3610 ccd2:23564 ccd3:26343 ccd4:22245 ccd5:22891 ccd6:30387 ccd7:25981 |
filter=Thin1 date-obs=2001-12-31T19:12:31 object=QR And roll_angle=247.893600464 |
|
pn | 56582 | 56583 | 56582 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd4:34243 |
filter=Thin1 date-obs=2001-12-31T18:52:40 object=QR And timedel=0.00 roll_angle=247.893600464 |
18 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 Sun Aug 12 09:55:06 2012
This data set was last accessed on Sun Aug 12 09:55:06 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0047940101
Position of field target = 0 19 50.00 21 56 54.0
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