The SWIFT BAT Software Guide Version 6.3 30 ... - HEASARC - Nasa
The SWIFT BAT Software Guide Version 6.3 30 ... - HEASARC - Nasa
The SWIFT BAT Software Guide Version 6.3 30 ... - HEASARC - Nasa
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138 APPENDIX D. <strong>BAT</strong> SOFTWARE TOOL REFERENCE<br />
parameter, and quantization can be disabled. <strong>The</strong> default quantization (7 bits of noise) should be<br />
more than enough to preserve all image features.<br />
D.8.4 PARAMETERS<br />
infile [filename ]<br />
Input file name containing <strong>BAT</strong> detector plane image. If pcodemap is ‘YES’, then the contents<br />
of the map are ignored, but the keywords from the map file are used to select the calibration<br />
files from CALDB. Thus, using a detector enable map or a quality map is appropriate in that<br />
case. Avoid using the CFITSIO syntax to select image extensions; use the ‘rows’ parameter<br />
instead.<br />
outfile [filename ]<br />
Output sky image or partial coding map file name.<br />
attitude = “NONE” [string ]<br />
Swift attitude file name. If NONE is given, then a celestial coordinate system cannot be<br />
assigned to the image.<br />
(aperture = “CALDB:FLUX”)[filename ]<br />
<strong>BAT</strong> aperture map file name, which contains the coded mask pattern and alignment parameters.<br />
If the CALDB database is set up, then CALDB can also be specified. If several<br />
aperture types are available in the CALDB, the user can specify CALDB:apertype. Valid<br />
values of apertype are currently: FLUX or DETECTION, for apertures optimized for flux<br />
reproducibility or detection sensitivity, respectively.<br />
(detmask = “NONE”) [string ]<br />
Name of a detector quality map file. This should be an image file with the same dimensions<br />
as the focal plane map. A pixel value of 0 indicates the detector is enabled for imaging, and<br />
a non-zero value indicates disabled. A default value of NONE implies all detectors are on,<br />
except for the <strong>BAT</strong> detector gap regions.<br />
(bkgfile = “NONE”) [string ]<br />
Name of a file containing background image data to be subtracted from the input. A value<br />
of NONE indicates no subtraction should be performed.<br />
(bkgvarmap=“NONE”) [string ]<br />
Optional output file name for the theoretical Poisson background fluctuation map. This map<br />
will be either the standard deviation map or the variance map depending on the value of<br />
bkgvartype. NOTE: <strong>The</strong> input map must not be cleaned for the theoretical map to be<br />
computed properly. A value of NONE indicates no fluctuation maps should be created. A<br />
value of APPEND indicates that each fluctuation map should be appended to the output file<br />
given by ‘outfile’.<br />
(bkgvartype=“STDDEV”) [string ]<br />
Type of output fluctuation map. Valid values are: STDDEV, for a standard deviation map;<br />
or VARIANCE, for a variance map.