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 | 10941 | 10879 | 10878 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:3929 ccd2:1603 ccd3:6254 ccd4:2053 ccd5:1650 ccd6:1961 ccd7:1574 |
filter=Medium date-obs=2003-01-29T05:00:02 object=PSR 1259-63/SS2883 roll_angle=120.731674194 |
|
mos2 | 10957 | 10894 | 10893 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:3974 ccd2:1603 ccd3:1826 ccd4:5265 ccd5:1922 ccd6:2314 ccd7:1798 |
filter=Medium date-obs=2003-01-29T05:00:01 object=PSR 1259-63/SS2883 roll_angle=120.731674194 |
14 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 Sun Jun 9 17:32:05 2013
This data set was last accessed on Sun Jun 9 17:32:05 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0092821201
Position of field target = 13 2 47.68 -63 50 8.6
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