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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D.15. <strong>BAT</strong>MASKWTIMG 167<br />
(aperture = “CALDB”)[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, DETECTION, or MASK EDGES; for apertures<br />
optimized for flux reproducibility, detection sensitivity, or for the shadow of the edge of the<br />
mask, respectively.<br />
(coord type = “sky”) [string ]<br />
Method of specifying the source coordinates. It should be one of: “sky”; “tanxy” (coordinates<br />
expressed in tangent-plane coordinates); “cartesian” (source at cartesian position in <strong>BAT</strong><br />
coordinates); “unit” (unit vector direction in <strong>BAT</strong> coordinates); “fswlonlat” (flight software<br />
phi and theta); “grmclonlat” (source at simulator longitude and latitude). All coordinate<br />
types but the first are specified in the instrument coordinate system.<br />
(time = 0) [real ]<br />
Time associated with the mask weighted image. When coordinates are used, it is also possible<br />
for the attitude to change as a function of time. Specify the mission elapsed time of interest<br />
with this parameter. A value of 0 (the default) indicates to use the first row of the attitude<br />
file, or the time in ‘infile’ if it is present. Ignored for non-sky coordinate systems.<br />
(rebalance = YES) [boolean ]<br />
If YES, then the mask weight map will be adjusted so that its additive mean is zero. If NO,<br />
then, the map will be written unadjusted.<br />
(bat z = 0) [real ]<br />
Position of the source in <strong>BAT</strong> Z coordinates, if coord type is “cartesian” (in units of cm).<br />
(incatalog = “NONE”) [string ]<br />
Input source catalog containing source positions. <strong>The</strong> catalog should contain one row per<br />
source. A value of NONE indicates that the source coordinates should be taken from the<br />
command line.<br />
(racol = “RA OBJ”) [string ]<br />
Column name of the first coordinate value in the input catalog, typically right ascension.<br />
(deccol = “DEC OBJ”) [string ]<br />
Column name of the second coordinate value in the input catalog, typically declination.<br />
(namecol = “NAME”) [string ]<br />
Column name of the source name in the input catalog. This value is written to the output<br />
keyword named ‘OBJECT’. If NONE is specified, then this column is ignored.<br />
(catnumcol = “CATNUM”) [string ]<br />
Column name of the source catalog number in the input catalog. This value is written to the<br />
output keyword named ‘CATNUM’. If NONE is specified, then this column is ignored.<br />
(outtype = “WEIGHTS”) [string ]<br />
Type of output map (one of WEIGHTS, ZERO or NONZERO). For ZERO, the test (weight<br />
== 0) is performed on each pixel; for NONZERO, the test (weight != 0) is performed.<br />
(1=true; 0=false).