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 | 21442 | 21440 | 17472 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd2:14762 ccd3:18531 ccd4:14560 ccd5:15725 ccd6:17433 ccd7:14201 |
filter=Thick date-obs=2002-02-22T23:29:57 object=Sigma2 CrB roll_angle=97.5123062134 |
|
mos2 | 21417 | 17917 | 12254 | 1.00 | 4.35 | 0/0 | Yes | orig clean | ccd1:276074 ccd2:76768 ccd3:86547 ccd4:69421 ccd5:75188 ccd6:97455 ccd7:81669 |
filter=Medium date-obs=2002-02-22T23:29:59 object=Sigma2 CrB roll_angle=97.5123062134 |
13 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 May 19 03:12:04 2013
This data set was last accessed on Sun May 19 03:12:04 2013
Current user = xassist on x3.localdomain
Number of fields in memory = 1
Current field being processed = xmm0111470301
Position of field target = 16 14 41.70 33 51 35.0
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