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author | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
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committer | Joseph Hunkeler <jhunkeler@gmail.com> | 2015-07-08 20:46:52 -0400 |
commit | fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4 (patch) | |
tree | bdda434976bc09c864f2e4fa6f16ba1952b1e555 /math/curfit/cvfitd.x | |
download | iraf-linux-fa080de7afc95aa1c19a6e6fc0e0708ced2eadc4.tar.gz |
Initial commit
Diffstat (limited to 'math/curfit/cvfitd.x')
-rw-r--r-- | math/curfit/cvfitd.x | 45 |
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diff --git a/math/curfit/cvfitd.x b/math/curfit/cvfitd.x new file mode 100644 index 00000000..bd4f9e83 --- /dev/null +++ b/math/curfit/cvfitd.x @@ -0,0 +1,45 @@ +# Copyright(c) 1986 Association of Universities for Research in Astronomy Inc. + +include <math/curfit.h> + +include "dcurfitdef.h" + +# CVFIT -- Procedure to add a set of points to the normal equations. +# The inner products of the basis functions are calculated and +# accumulated into the CV_ORDER(cv) by CV_NCOEFF(cv) matrix MATRIX. +# The main diagonal of the matrix is stored in the first row of +# MATRIX followed by the remaining non-zero diagonals. This method +# of storage is particularly efficient for the large symmetric +# banded matrices produced during spline fits. The inner product +# of the basis functions and the data ordinates are stored in the +# CV_NCOEFF(cv)-vector VECTOR. The array LEFT is +# used for the indices describing which elements of MATRIX and VECTOR are +# to receive the inner products. After accumulation is complete +# the Cholesky factorization of MATRIX is calculated and stored +# in the CV_ORDER(cv) by CV_NCOEFF(cv) matrix CHOFAC. Finally +# the coefficients are calculated by forward and back substitution +# and placed in COEFF. + +procedure dcvfit (cv, x, y, w, npts, wtflag, ier) + +pointer cv # curve descriptor +double x[npts] # array of abcissa +double y[npts] # array of ordinates +double w[npts] # array of weights +int npts # number of data points +int wtflag # type of weighting +int ier # error code + + +begin + + # zero the appropriate arrays + call dcvzero (cv) + + # enter data points + call dcvacpts (cv, x, y, w, npts, wtflag) + + # solve the system + call dcvsolve (cv, ier) + +end |