PURIFY(26)

NAME
purify - Reconstruct images from radio interferometers using PADMM

SYNOPSIS
purify [CONFIGFILE]

DESCRIPTION
PURIFY is a tool for radio interferometric imaging including file handling (for both visibilities and fits files), implementation of the measurement operator and set-up of the different optimization problems used for image deconvolution.

The code is given for educational purpose. The code is in beta and still under development.

OPTIONS
purify only requires a config yaml file with all the details needed to run it. Details about how to create such file are available in the source or online at https://github.com/astro-informatics/purify/blob/development/data/config/config.yaml

AUTHORS
PURIFY was initially created by Rafael Carrillo, Jason McEwen and Yves Wiaux but major contributions have since been made by a number of others. The full list of contributors is as follows: Rafael E. Carrillo, Jason D. McEwen, Yves Wiaux, Luke Pratley, Mayeul d'Avezac, Ilektra Christidi, Roland Guichard and David Perez-Suarez.

BUGS
If you have any questions or comments, feel free to contact Rafael Carrillo or Jason McEwen, or add an issue in the issue tracker https://github.com/astro-informatics/purify/issues

LICENSE
PURIFY Copyright (C) 2013 Rafael Carrillo, Jason McEwen, Yves Wiaux

This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 2 of the License, or (at your option) any later version.

This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details.