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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /math/iminterp/doc/asigrl.hlp | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/iminterp/doc/asigrl.hlp')
-rw-r--r-- | math/iminterp/doc/asigrl.hlp | 40 |
1 files changed, 40 insertions, 0 deletions
diff --git a/math/iminterp/doc/asigrl.hlp b/math/iminterp/doc/asigrl.hlp new file mode 100644 index 00000000..4c3087bb --- /dev/null +++ b/math/iminterp/doc/asigrl.hlp @@ -0,0 +1,40 @@ +.help asigrl Dec98 "Image Interpolator Package" +.ih +NAME +asigrl -- integrate interpolant from a to b +.ih +SYNOPSIS +integral = asigrl (asi, a, b) + +.nf + pointer asi #I interpolant descriptor + real a #I lower limit for integral, 1 <= a <= npix + real b #I upper limit for integral, 1 <= b <= npix +.fi +.ih +ARGUMENTS +.ls asi +Pointer to the sequential interpolant descriptor structure. +.le +.ls a +Lower limit to the integral, where 1 <= a <= npix. +.le +.ls b +Upper limit to the integral, where 1 <= b <= npix. +.le +.ih +DESCRIPTION +The integral is calculated assuming that the interior polynomial, sinc, and +drizzle interpolants are stored as the data points, and that the spline +interpolant is stored as an array of B-spline coefficients. + +The integral of the sinc interpolant is computed by dividing the integration +interval into a number of equal size subintervals which are at most one pixel +wide. The integral of each subinterval is the central value times the interval +width. The look-up table sinc interpolant is not supported and defaults to +the sinc interpolant. +.ih +NOTES +ASIINIT or ASISINIT and ASIFIT must be called before using ASIGRL. +.ih +SEE ALSO |