SINFONI Pipeline Reference Manual  2.6.0
sinfo_new_nst.h
1 #ifndef SINFO_NEW_NST_H
2 #define SINFO_NEW_NST_H
3 /*
4  * This file is part of the ESO SINFONI Pipeline
5  * Copyright (C) 2004,2005 European Southern Observatory
6  *
7  * This program is free software; you can redistribute it and/or modify
8  * it under the terms of the GNU General Public License as published by
9  * the Free Software Foundation; either version 2 of the License, or
10  * (at your option) any later version.
11  *
12  * This program is distributed in the hope that it will be useful,
13  * but WITHOUT ANY WARRANTY; without even the implied warranty of
14  * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
15  * GNU General Public License for more details.
16  *
17  * You should have received a copy of the GNU General Public License
18  * along with this program; if not, write to the Free Software
19  * Foundation, 51 Franklin St, Fifth Floor, Boston, MA 02111-1307 USA
20  */
21 /*****************************************************************************
22 * E.S.O. - VLT project
23 *
24 * "@(#) $Id: sinfo_new_nst.h,v 1.7 2007-09-21 14:49:00 amodigli Exp $"
25 *
26 * who when what
27 * -------- -------- ----------------------------------------------
28 * amodigli 17/09/03 created
29 */
30 
31 /************************************************************************
32  * new_nsh.h
33  * Result of a north-south test exposure are 32 continuum spectra of a
34  * pinhole that means one spectrum in each slitlet at the same spatial
35  * position.
36  * Each spectrum is fitted in sp[atial direction by a Gaussian to get the
37  * sub-pixel positions for each row.
38  *
39  * Then the distances are determined in each row and averaged
40  *
41  * Result: are distances of each slitlet from each other => 31 values stored
42  * in an ASCII file this Python script needs a frame of a pinhole source with
43  * a continuous spectrum, that is shifted exactly perpendicular to the
44  * slitlets. It fits the spectra in spatial direction by a Gaussian fit
45  * function and therefore determines the sub-pixel position of the source.
46  *
47  * Then the distances of the slitlets from each other are determined and
48  * saved in an ASCII list.
49  *
50  *----------------------------------------------------------------------
51  */
52 
53 /*
54  * header files
55  */
56 #include <cpl.h>
57 #include "sinfo_msg.h"
58 /*----------------------------------------------------------------------------
59  * Function ANSI C prototypes
60  *--------------------------------------------------------------------------*/
61 
62 /*----------------------------------------------------------------------------
63  Function : sinfo_nst()
64  In : ini_file: file name of according .ini file
65  Out : integer (0 if it worked, -1 if it doesn't)
66  Job :
67 
68  * Result of a north-south test exposure are 32 continuum spectra of a
69  * pinhole that means one spectrum in each slitlet at the same spatial
70  * position.
71  * Each spectrum is fitted in sp[atial direction by a Gaussian to get the
72  * sub-pixel positions for each row.
73  *
74  * Then the distances are determined in each row and averaged
75 
76 
77  ---------------------------------------------------------------------------*/
78 int
79 sinfo_new_nst (const char* plugin_id,
80  cpl_parameterlist* config,
81  cpl_frameset* set,
82  cpl_frameset* ref_set) ;
83 
84 
85 #endif
86 
87 /*--------------------------------------------------------------------------*/