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.14. <strong>BAT</strong>MASKWTEVT 163<br />
(distance = 1.0e7) [real ]<br />
Default bat z position if bat z is zero (centimeters).<br />
(maskoffx = 0.0) [real ]<br />
Translational offset to apply to the mask along the <strong>BAT</strong> X coordinate from its nominal design<br />
position.<br />
(maskoffy = 0.0) [real ]<br />
Translational offset to apply to the mask along the <strong>BAT</strong> Y coordinate from its nominal design<br />
position.<br />
(maskoffz = 0.0) [real ]<br />
Translational offset to apply to the mask along the <strong>BAT</strong> Z coordinate from its nominal design<br />
position.<br />
(maskthickness = INDEF) [string ]<br />
Thickness of the lead mask tiles in centimeters. Normally this will be set to INDEF, which<br />
reads the mask thickness from the aperture file. A thickness of 0 cm is permitted.<br />
(distfile=CALDB) [string ]<br />
<strong>The</strong> ‘distfile’ parameter should point to a FITS file containing an MxNx2 image (or CALDB<br />
to use the default instrument correction in the calibration database). <strong>The</strong> two planes of the<br />
image are the non-linear distortion of the <strong>BAT</strong> “plate scale” as a function of position in the<br />
sky image. <strong>The</strong> values are offsets in tangent plane coordinates (IMX,IMY), and therefore<br />
unitless. <strong>The</strong> first plane of the image cube is the IMX offset, and the second plane is the<br />
IMY offset. <strong>The</strong> sense of the offset is (TRUE-APPARENT), i.e. for a measured position in<br />
tangent plane coordinates, the offset values should be *added* to arrive at the true position<br />
in tangent plane coordinates. <strong>The</strong> images are low-resolution versions of the <strong>BAT</strong> field of view<br />
in instrumental sky coordinates, and are meant to be interpolated to the desired sampling.<br />
<strong>The</strong> WCS keywords must specify the image coordinate systems.<br />
(buffersize = 32768) [integer ]<br />
Size of internal event buffer for processing.<br />
(subpixsize = 0.02) [real ]<br />
Size of detector subpixels used in computing mask weighting, in centimeters. Can be no larger<br />
than 0.02 cm.<br />
(teldef = “CALDB”) [string ]<br />
<strong>BAT</strong> instrument telescope description file, which defines instrument-to-spacecraft alignments.<br />
Must be specified when celestial coordinates are provided. If the CALDB database is set up,<br />
then CALDB can also be specified.<br />
(origin z = 0) [real ]<br />
For ground testing with a near-field source. <strong>The</strong> position of the origin of coordinates (in cm),<br />
to which the source position is referred.<br />
(maskwtswgain = 0.04) [real ]<br />
Mask weight technique software gain correction factor. When corrections=maskwt, the<br />
weights are divided by (1+maskwtswgain). This is correction is software algorithm dependent<br />
and not intended to be changed by the user.