SINFONI Pipeline Reference Manual
2.6.0
sinfoni
sinfo_new_stdstar.h
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#ifndef SINFO_NEW_STDSTAR_H
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#define SINFO_NEW_STDSTAR_H
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/*
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* This file is part of the ESO SINFONI Pipeline
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* Copyright (C) 2004,2005 European Southern Observatory
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*
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* This program is free software; you can redistribute it and/or modify
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* it under the terms of the GNU General Public License as published by
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* the Free Software Foundation; either version 2 of the License, or
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* (at your option) any later version.
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*
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* This program is distributed in the hope that it will be useful,
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* but WITHOUT ANY WARRANTY; without even the implied warranty of
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* MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
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* GNU General Public License for more details.
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*
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* You should have received a copy of the GNU General Public License
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* along with this program; if not, write to the Free Software
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* Foundation, 51 Franklin St, Fifth Floor, Boston, MA 02111-1307 USA
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*/
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/*******************************************************************************
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* E.S.O. - VLT project
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*
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* "@(#) $Id: sinfo_new_stdstar.h,v 1.11 2007-09-21 14:13:43 amodigli Exp $"
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*
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* who when what
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* -------- -------- ----------------------------------------------
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* schreib 06/05/03 created
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*/
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/************************************************************************
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* sinfo_new_stdstar.h
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* routines to create a data cube
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*----------------------------------------------------------------------
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*/
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/*
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* header files
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*/
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#include <cpl.h>
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#include "sinfo_msg.h"
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#include <sinfo_standstar_cfg.h>
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/*----------------------------------------------------------------------------
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* Function ANSI C prototypes
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*--------------------------------------------------------------------------*/
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/*----------------------------------------------------------------------------
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Function : sinfo_new_stdstar()
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In : ini_file: file name of according .ini file
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Out : integer (0 if it worked, -1 if it doesn't)
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Description : this routine does the optimal extraction of a spectrum
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of an already reduced data cube of a standard star
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observation. Additionally, a conversion factor from
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mag to counts/sec can be determined if the magnitude
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of the standard star is known.
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This is done for a number of jittered data cubes and
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the results are averaged by rejecting the extreme
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values
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---------------------------------------------------------------------------*/
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int
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sinfo_new_stdstar (
const
char
* plugin_id,
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cpl_parameterlist* config,
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cpl_frameset* sof,cpl_frameset* ref_set) ;
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#endif
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/*--------------------------------------------------------------------------*/
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