Detector | Exposure (Original/Cleaned) | Image binning | Plate scale ("/pixel) | Bgd. level (orig/cleaned, counts/sq. arcmin/s) | GTI file | Bgd. light curves | Roll angle | CCD counts | Extra info |
---|---|---|---|---|---|---|---|---|---|
ccd7 | 606 | 606 | 1.00 | 0.49 | 3.7e+02/3.7e+02 | Yes | orig clean | |||
acis | 606 | 606 | 4.00 | 1.97 | 0/0 | Yes | orig clean | ccd7:1694753 |
datamode=GRADED readmode=TIMED gainfile=acisD2000-01-29gainN0005.fits CCD Temp=-119 object=Crab Nebula firstrow=39 nrows=300 date-obs=2010-09-28T05:05:57 roll_angle=92.3926246758 timedel=0.24 (1/14 readout) CIAO_version=8.3.2.1 |
103 source(s) in memory Iteration: 2 Images: |ccd7 |acis |
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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
CIAO version = 4.3.0
XAssist version = 1.000
numpy version = 1.3.0
Pyfits version = 2.1.1
XAssist originally started on this data set at Mon Sep 26 07:56:07 2011
This data set was last accessed on Mon Sep 26 07:56:07 2011
Current user = xassist on xassist.localdomain
Number of fields in memory = 1
Current field being processed = acisf13139
Position of field target = 5 34 31.60 22 0 56.4
Current telescope = chandra
Current detector = acis
Processing mode = proc
Processing status = OK
Detection method = wavelet
Batch processing enabled
Place data, logs, etc. in field subdirectories
Image analysis will be over range of allowed energies
Will analyze each ccd separately
Will skip analysis of CCD 8
Log files: processing messages |error messages |all messages (very detailed) |source logs