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 | 55207 | 55196 | 55196 | 1.00 | 4.35 | 0.0064/0.0064/0.0064 | Yes | orig clean | ccd1:361895 ccd2:9636 ccd3:23115 ccd4:11050 ccd5:10411 ccd6:13676 ccd7:9907 |
filter=Thick date-obs=2000-11-02T14:20:13 object=Vela X-1 roll_angle=98.1096191406 |
|
mos2 | 43071 | 43070 | 43068 | 1.00 | 4.35 | 0.0036/0.0036/0.0036 | Yes | orig clean | ccd1:409249 ccd2:8390 ccd3:9718 ccd4:7367 ccd5:12563 ccd6:11320 ccd7:9020 |
filter=Thick date-obs=2000-11-02T17:42:27 object=Vela X-1 roll_angle=98.1096191406 |
30 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 = 6.11
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 Dec 18 00:10:05 2011
This data set was last accessed on Sun Dec 18 00:10:05 2011
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111030101
Position of field target = 9 2 6.86 -40 33 16.9
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