#ifndef SINFO_NEW_CUBES_BUILD_H #define SINFO_NEW_CUBES_BUILD_H /* * This file is part of the ESO SINFONI 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 */ /******************************************************************************* * E.S.O. - VLT project * * "@(#) $Id: sinfo_new_cubes_build.h,v 1.11 2007-06-06 07:10:45 amodigli Exp $" * * who when what * -------- -------- ---------------------------------------------- * schreib 06/05/03 created */ /************************************************************************ * sinfo_cubes_build.h * routines to create a data cube *---------------------------------------------------------------------- */ /* * header files */ #include #include #include "sinfo_msg.h" /*---------------------------------------------------------------------------- * Function ANSI C prototypes *--------------------------------------------------------------------------*/ /*---------------------------------------------------------------------------- @name sinfo_new_cubes_build() @param plugin_id name of recipe plugin @param config input parameter list @param sof input frameset @param procatg @param frame_index index of processed frame @return integer (0 if it worked, -1 if it doesn't) @doc this routine does the resampling of an offset-corrected, flatfielded, bad pixel corrected and eventually interleaved data frame. Additionally, an intensity calibration is carried through by using a standard star or a black body measurement. The spectral features of the flatfield halogen lamp are corrected. Afterwards a data cube is created out of the resampled image. It is the users choice to use either the fitted sinfo_edge positions of the slitlets or the distances of the slitlets gained from a north-south-test. ---------------------------------------------------------------------------*/ int sinfo_new_cubes_build (const char* plugin_id, cpl_parameterlist* config, cpl_frameset* sof, const char* procatg, const int frame_index) ; #endif /*!SINFO_CUBES_BUILD_H*/ /*--------------------------------------------------------------------------*/