/*
 * This file is part of the ESO UVES Pipeline
 * Copyright (C) 2004,2005 European Southern Observatory
 *
 * 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.
 *
 * You should have received a copy of the GNU General Public License
 * along with this program; if not, write to the Free Software
 * Foundation, 51 Franklin St, Fifth Floor, Boston, MA  02111-1307  USA
 */
/*
 * $Author: jtaylor $
 * $Date: 2012-11-19 09:16:16 $
 * $Revision: 1.4 $
 * $Name: not supported by cvs2svn $
 * $Log: not supported by cvs2svn $
 * Revision 1.3  2010/09/24 09:31:29  amodigli
 * put back QFITS dependency to fix problem spot by NRI on FIBER mode (with MIDAS calibs) data
 *
 * Revision 1.1  2007/07/27 08:27:51  amodigli
 * added to repository
 *
 * Revision 1.1  2007/07/27 06:44:09  amodigli
 * added to repository
 *
 */

#ifndef FLAMES_LFIT_H
#define FLAMES_LFIT_H

#ifdef HAVE_CONFIG_H
#  include <config.h>
#endif

#include <flames_uves.h>
/* 
   ------------------------------------------------
   public C functions from Numerical Recipes
   modified for their use within the MIDAS environment
   ------------------------------------------------
*/
void 
lfit(double x[], double y[], double sig[], int32_t ndat, double a[], 
      int ia[], int ma, double **covar, double *chisq, 
      void (*funcs)(double, double [], int));


#endif
