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 | 32194 | 32194 | 31739 | 1.00 | 4.35 | 0.0023/0.0023/0.002 | Yes | orig clean | ccd2:5690 ccd3:7992 ccd4:5819 ccd5:5552 ccd6:6753 ccd7:5671 |
filter=Medium date-obs=2001-02-13T19:44:23 object=VY Arietis roll_angle=252.526245117 |
|
mos2 | 32798 | 32798 | 32477 | 1.00 | 4.35 | 0.0027/0.0027/0.0025 | Yes | orig clean | ccd1:128950 ccd2:5806 ccd3:6526 ccd4:5615 ccd5:5850 ccd6:8006 ccd7:5909 |
filter=Medium date-obs=2001-02-13T19:33:56 object=VY Arietis roll_angle=252.526245117 |
19 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 Jan 1 09:55:06 2012
This data set was last accessed on Sun Jan 1 09:55:06 2012
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111490401
Position of field target = 2 48 43.70 31 6 54.7
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