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 | 17888 | 17888 | 17888 | 1.00 | 4.35 | 0.0017/0.0017/0.0017 | Yes | orig clean | ccd2:2413 ccd3:3001 ccd4:2336 ccd5:2586 ccd6:3572 ccd7:2314 |
filter=Medium date-obs=2002-06-30T03:02:06 object=Ton S 180 roll_angle=66.5301055908 |
|
mos2 | 18153 | 18153 | 18153 | 1.00 | 4.35 | 0.002/0.002/0.002 | Yes | orig clean | ccd1:35749 ccd2:2857 ccd3:2915 ccd4:2288 ccd5:2422 ccd6:3117 ccd7:3019 |
filter=Medium date-obs=2002-06-30T03:02:12 object=Ton S 180 roll_angle=66.5301055908 |
|
pn | 18000 | 18000 | 18000 | 1.00 | 4.35 | 0.047/0.047/0.047 | Yes | orig clean | ccd4:111995 |
filter=Medium date-obs=2002-06-30T03:06:41 object=Ton S 180 timedel=0.00 roll_angle=66.5301055908 |
31 source(s) in memory Iteration: 2 Images: |mos1 |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 Nov 27 07:53:16 2011
This data set was last accessed on Sun Nov 27 07:53:16 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0110890701
Position of field target = 0 57 20.00 -22 22 59.0
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