CONTRIBUTORS

Copyright 2013 Joshua C. Dolence, Charles F. Gammie, Monika Mo\'scibrodzka, and Po Kin Leung

All other modifications including 3D support, HARMPI, alpha GPU acceleration with CUDA and more were added by Rodrigo Nemmen, Matheus Tavares and others (see full list of contributors in github).

GRMONTY  version 1.0   (released February 1, 2013)
=====================

This file is part of GRMONTY.  GRMONTY v1.0 is a program that calculates the emergent spectrum from a model using a Monte Carlo technique. This version of GRMONTY is configured to use input files from the HARM code available on the same site.   It assumes that the source is a plasma near a black hole described by Kerr-Schild coordinates that radiates via thermal synchrotron and inverse compton scattering.
    
    You are morally obligated to cite the following paper in any
    scientific literature that results from use of any part of GRMONTY:

    Dolence, J.C., Gammie, C.F., Mo\'scibrodzka, M., \& Leung, P.-K. 2009,
        Astrophysical Journal Supplement, 184, 387

    Further, we strongly encourage you to obtain the latest version of 
    GRMONTY directly from our distribution website:
    http://rainman.astro.illinois.edu/codelib/

    GRMONTY 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.

    GRMONTY 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.

    You should have received a copy of the GNU General Public License
    along with GRMONTY; if not, write to the Free Software
    Foundation, Inc., 51 Franklin St, Fifth Floor, Boston, MA  02110-1301  USA