Description:
This routine performs two tasks:
Invocation
CALL
SCULIB_WTFN_REGRID_1 (DIAMETER, WAVELENGTH, WEIGHT, IN_DATA, X, Y, NPIX, PIXSPACE, NI,
NJ, ICEN, JCEN, AV_WEIGHT, SCRATCH, STATUS)
Arguments
DIAMETER = REAL (Given)
Diameter of telescope
WAVELENGTH = REAL (Given)
Wavelength of the observation
WEIGHT
= REAL (Given)
The weight of the input dataset.
IN_DATA (NPIX) = REAL (Given)
The
input data values. (Used to define quality)
X( NPIX ) = DOUBLE PRECISION (Given)
The x coordinates of the input pixels
Y( NPIX ) = DOUBLE PRECISION (Given)
The y
coordinates of the input pixels
NPIX = INTEGER (Given)
the number of input pixels
PIXSPACE = DOUBLE PRECISION (Given)
the pixel spacing of the output pixels
NI =
INTEGER (Given)
The number of output pixels in the x direction
NJ = INTEGER (Given)
The number of output pixels in the y direction
ICEN = INTEGER (Given)
the x index
of the centre of the output array
JCEN = INTEGER (Given)
the y index of the centre
of the output array
AV_WEIGHT (NI, NJ) = REAL (Given and Returned)
Given as a
workspace array
SCRATCH (NI, NJ) = INTEGER (Returned)
Temporary workspace.
STATUS = INTEGER (Given and Returned)
The global status.
Copyright
Copyright
©1995,1996,1997,1998,1999 Particle Physics and Astronomy Research Council. All Rights Reserved.