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 |
---|---|---|---|---|---|---|---|---|---|
ccd3 | 55613 | 55613 | 1.00 | 0.49 | 0.0069/0.0069 | Yes | orig clean | |||
acis | 55613 | 55613 | 4.00 | 1.97 | 0/0 | Yes | orig clean | 264.9 | ccd3:11063 |
datamode=VFAINT readmode=TIMED gainfile=acisD2000-01-29gain_ctiN0006.fits CCD Temp=-120 object=PSR J0538+2817 firstrow=865 nrows=160 date-obs=2006-01-20T14:29:41 roll_angle=265.21004651 timedel=0.54 (1/6 readout) CIAO_version=7.6.6 |
3 source(s) in memory Iteration: 2 Images: |ccd3 |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 Sun Sep 25 23:06:06 2011
This data set was last accessed on Sun Sep 25 23:06:06 2011
Current user = xassist on xassist.localdomain
Number of fields in memory = 1
Current field being processed = acisf05538
Position of field target = 5 38 25.05 28 17 8.8
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