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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).

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