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 |
---|---|---|---|---|---|---|---|---|---|
ccd2 | 158025 | 158025 | 1.00 | 0.49 | 0.0054/0.0054 | Yes | orig clean | |||
ccd3 | 158021 | 158021 | 1.00 | 0.49 | 0.0057/0.0057 | Yes | orig clean | |||
ccd5 | 158025 | 158025 | 1.00 | 0.49 | 0.017/0.017 | Yes | orig clean | |||
ccd6 | 158018 | 158018 | 1.00 | 0.49 | 0.0095/0.0095 | Yes | orig clean | |||
ccd7 | 158025 | 158025 | 1.00 | 0.49 | 0.33/0.33 | Yes | orig clean | |||
acis | 158025 | 158025 | 4.00 | 1.97 | 0/0 | Yes | orig clean | ccd2:69055 ccd3:66539 ccd5:192569 ccd6:111474 ccd7:6873537 ccd8:98546 |
datamode=FAINT readmode=TIMED gainfile=acisD2000-01-29gain_ctiN0006.fits CCD Temp=-119 object=Kepler's Supernova Remnant firstrow=1 nrows=1024 date-obs=2006-05-05T19:18:18 roll_angle=89.5192157952 timedel=3.24 (full readout) CIAO_version=7.6.7.2 |
460 source(s) in memory Iteration: 2 Images: |ccd2 |ccd3 |ccd5 |ccd6 |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 Sun Sep 25 01:33:11 2011
This data set was last accessed on Sun Sep 25 01:33:11 2011
Current user = xassist on xassist.localdomain
Number of fields in memory = 1
Current field being processed = acisf06716
Position of field target = 17 30 42.00 -21 28 60.0
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