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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/surfit/iscoeff.x | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'math/surfit/iscoeff.x')
-rw-r--r-- | math/surfit/iscoeff.x | 37 |
1 files changed, 37 insertions, 0 deletions
diff --git a/math/surfit/iscoeff.x b/math/surfit/iscoeff.x new file mode 100644 index 00000000..f656e7e6 --- /dev/null +++ b/math/surfit/iscoeff.x @@ -0,0 +1,37 @@ +# Copyright(c) 1986 Association of Universities for Research in Astronomy Inc. + +include "surfitdef.h" + +# ISCOEFF -- Procedure to fetch the number and magnitude of the coefficients. +# If the surface type is a bicubic spline or polynomials with cross terms +# then the number of coefficients is SF_NXCOEFF(sf) * SF_NYCOEFF(sf) and +# the coefficient of B(i,x) * B(j,y) will be stored in element +# (i - 1) * SF_NYCOEFF(sf) + j of the array coeff. Otherwise the number +# of coefficients will be (SF_NXCOEFF(sf) + SF_NYCOEFF(sf) - 1), and +# the SF_NYCOEFF(sf) y coefficients will be output first followed by +# the (SF_NXCOEFF(sf) - 1) x coefficients. + +procedure iscoeff (sf, coeff, ncoeff) + +pointer sf # pointer to the surface fitting descriptor +real coeff[ARB] # the coefficients of the fit +int ncoeff # the number of coefficients + +int i +pointer cptr + +begin + # calculate the number of coefficients + if (SF_XTERMS(sf) == NO) { + ncoeff = SF_NXCOEFF(sf) + SF_NYCOEFF(sf) - 1 + call amovr (COEFF(SF_COEFF(sf)), coeff, SF_NYCOEFF(sf)) + cptr = SF_COEFF(sf) + SF_NYCOEFF(sf) + do i = SF_NYCOEFF(sf) + 1, ncoeff { + coeff[i] = COEFF(cptr) + cptr = cptr + SF_NYCOEFF(sf) + } + } else { + ncoeff = SF_NXCOEFF(sf) * SF_NYCOEFF(sf) + call amovr (COEFF(SF_COEFF(sf)), coeff, ncoeff) + } +end |