/*
 * 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  2007/07/30 06:49:58  amodigli
 * added to repository (removed from flames_uves.h)
 *
 * Revision 1.1  2007/07/27 06:44:09  amodigli
 * added to repository
 *
 */

#ifndef FLAMES_DO_STANDARD_H
#define FLAMES_DO_STANDARD_H

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

#include <flames_uves.h>


/* the following function performs the actual standard extraction on a frame */
flames_err 
dostandard(flames_frame *ScienceFrame, 
           orderpos *Order, 
       allflats *Shifted_FF, 
           frame_mask **mask, 
       double ***pfibrecentre, 
           double phalfwinsize, 
       int32_t realfirstorder, 
           int32_t reallastorder);


#endif
