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 | 48054 | 48054 | 48050 | 1.00 | 4.35 | 0.0026/0.0026/0.0026 | Yes | orig clean | ccd2:10210 ccd3:12235 ccd4:11074 ccd5:10487 ccd7:10029 |
filter=Thin1 date-obs=2007-10-20T06:36:52 object=VV Pup roll_angle=97.0879745483 |
|
mos2 | 47999 | 47926 | 47926 | 1.00 | 4.35 | 0.0025/0.0025/0.0025 | Yes | orig clean | ccd2:10667 ccd3:11160 ccd4:8589 ccd5:9804 ccd6:11484 ccd7:10175 |
filter=Thin1 date-obs=2007-10-20T06:36:52 object=VV Pup roll_angle=97.0879745483 |
55 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 Tue Jan 3 05:31:04 2012
This data set was last accessed on Tue Jan 3 05:31:04 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0501750801
Position of field target = 8 15 6.70 -19 3 15.0
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