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/*
* 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
*/
#ifndef FLAMES_CORREL_H
#define FLAMES_CORREL_H
#ifdef HAVE_CONFIG_H
# include <config.h>
#endif
#include<flames_uves.h>
/*
The following function gives the optimal shift for the FF
in order to use them as a physical model for the perpendicular
shape of the PSF on the CCD by calculating the correlation
between Science Frame and FF.
*/
flames_err
correl(flames_frame *ScienceFrame,
allflats *SingleFF,
orderpos *Order,
double ytolerance,
int32_t maxshift,
double *finaldeltas,
frame_mask *finalmask,
char *outtabname);
#endif
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