NAME

       ficonv - obtaining and evaluating convolution transformations

SYNOPSIS

       ficonv [options] [-r <reference>] [-i <input>] [-o <output>]

DESCRIPTION

       The purpose of this program is twofold. First, using a reference and input FITS image, the
       program tries to figure out the best-fit convolution kernel which transforms the reference
       image  to  the  input  image.  The  convolution  kernel  solution  is saved as a separate,
       human-readable file. Second,  using  an  existing  such  kernel  solution  file,  `ficonv`
       convolves  the  reference  image and optionally co-adds an additional image to the result.
       The program figures out the desired mode (i.e. whether to fit a convolution kernel or  use
       an existing kernel solution to convolve an image) from the presence or lack of the command
       line options.

OPTIONS

   General options:
       -h, --help
              Gives general summary about the command line options.

       --long-help, --help-long
              Gives a detailed list of command line options.

       --wiki-help, --help-wiki, --mediawiki-help, --help-mediawiki
              Gives a detailed list of command line options in Mediawiki format.

       --version, --version-short, --short-version
              Gives some version information about the program.

       -r, --input-reference <image file>
              Name of the reference FITS image file.

       -i, --input <image file>
              Name of the input FITS image file (required only for kernel fitting).

       -k, --kernel <kernel set>
              List  of  kernel  bases  used  for  fitting  convolution  kernel.See  also  "Kernel
              specifications" below for the format of this <kernel set> argument.

       --input-kernel <file>
              Name of the file containing kernel bases. The kernel bases in this file should have
              no associated coefficients if convolution fitting is  done,  otherwise  the  kernel
              basis file must contain the convolution coefficients

       --output-kernel <file>
              Name  of  the  file  where  the  coefficients for the kernel bases are stored after
              convolution kernel fitting

       -o, -oc, --output, --output-convolved <image file>
              Name of the output file which is the reference  image  convolved  with  the  kernel
              solution  (which  can either be a previously fitted and now read from a file or the
              result of the current fit)

       --output-subtracted <image file>
              The difference between the input image and the convolved reference image.

       -a, --add-to <image file>
              This optionally specified file is added to the convolved image

       -M, --input-mask <fits>
              Input mask file to co-add to output image mask.

       -n, --iterations <iterations>
              Use an iterative fit with the rejection of the outlier pixels.The maximum number of
              iterations should be specified with this command line argument

       -s, --rejection-level <sigma>
              Rejection level in standard deviation units.

   Kernel specifications (each separated with a semi-colon,  ;"):"
       i/<spatial order>
              identity kernel (a.k.a. "flux term") with the specified order of polynomial spatial
              variations

       b/<spatial order>
              constant offset kernel (a.k.a. "background  term")  with  the  specified  order  of
              polynomial spatial variations

       d=<size>/<spatial order>
              discrete  kernel with the half-size of <size> and the specified order of polynomial
              spatial variations

       g=<size>,<sigma>,<order>/<spatial order>
              Gaussian kernel with the half-size of <size>, standard  deviation  of  <sigma>  and
              Hermite  basis  order  of  <order>,  with the specified order of polynomial spatial
              variations

REPORTING BUGS

       Report bugs to <apal@szofi.net>, see also http://fitsh.net/.

COPYRIGHT

       Copyright © 1996, 2002, 2004-2008, 2010-2015; Pal, Andras <apal@szofi.net>