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 | 5010 | 5010 | 1.00 | 0.49 | 0.0082/0.0082 | Yes | orig clean | |||
acis | 5010 | 5010 | 4.00 | 1.97 | 0/0 | Yes | orig clean | 182.7 | ccd7:3049 |
datamode=VFAINT readmode=TIMED gainfile=acisD2000-01-29gain_ctiN0006.fits CCD Temp=-120 object=6dF J0405204-364859 firstrow=1 nrows=1024 date-obs=2010-05-28T13:04:55 roll_angle=182.066123764 timedel=3.04 (full readout) CIAO_version=8.2.1 |
8 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 Oct 24 10:09:03 2011
This data set was last accessed on Mon Oct 24 10:09:03 2011
Current user = xassist on xassist.localdomain
Number of fields in memory = 1
Current field being processed = acisf11292
Position of field target = 4 5 20.40 -36 49 0.7
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