CR2RE Pipeline Reference Manual 1.6.7
irplib_stdstar.h
1/* $Id: irplib_stdstar.h,v 1.16 2013-02-27 10:37:52 llundin Exp $
2 *
3 * This file is part of the irplib package
4 * Copyright (C) 2002,2003 European Southern Observatory
5 *
6 * This program is free software; you can redistribute it and/or modify
7 * it under the terms of the GNU General Public License as published by
8 * the Free Software Foundation; either version 2 of the License, or
9 * (at your option) any later version.
10 *
11 * This program is distributed in the hope that it will be useful,
12 * but WITHOUT ANY WARRANTY; without even the implied warranty of
13 * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
14 * GNU General Public License for more details.
15 *
16 * You should have received a copy of the GNU General Public License
17 * along with this program; if not, write to the Free Software
18 * Foundation, Inc., 51 Franklin St, Fifth Floor, Boston, MA 02111-1307 USA
19 */
20
21/*
22 * $Author: llundin $
23 * $Date: 2013-02-27 10:37:52 $
24 * $Revision: 1.16 $
25 * $Name: not supported by cvs2svn $
26 */
27
28#ifndef IRPLIB_STDSTAR_H
29#define IRPLIB_STDSTAR_H
30
31/*-----------------------------------------------------------------------------
32 Includes
33 -----------------------------------------------------------------------------*/
34
35#include <cpl.h>
36
37/*-----------------------------------------------------------------------------
38 Defines
39 -----------------------------------------------------------------------------*/
40
41#define IRPLIB_STDSTAR_STAR_COL "STARS"
42#define IRPLIB_STDSTAR_TYPE_COL "SP_TYPE"
43#define IRPLIB_STDSTAR_RA_COL "RA"
44#define IRPLIB_STDSTAR_DEC_COL "DEC"
45#define IRPLIB_STDSTAR_CAT_COL "CATALOG"
46
47/* Maximum allowed distance [arc minutes] between observation and
48 catalogue coordinates */
49#define IRPLIB_STDSTAR_MAXDIST 2.0
50
51/* Magical value to indicate an invalid magnitude */
52#define IRPLIB_STDSTAR_NOMAG 99.0
53
54/* Use this limit in comparisons regarding an invalid magnitude */
55#define IRPLIB_STDSTAR_LIMIT (IRPLIB_STDSTAR_NOMAG-1.0)
56
57/*-----------------------------------------------------------------------------
58 Function prototypes
59 -----------------------------------------------------------------------------*/
60
61cpl_error_code
62irplib_stdstar_write_catalogs(cpl_frameset *, const cpl_frameset *,
63 const char *, const char *, const char *,
64 const char *, const char *,
65 cpl_table * (*)(const char *));
66cpl_table * irplib_stdstar_load_catalog(const char *, const char *);
67cpl_error_code irplib_stdstar_check_columns_exist(const cpl_table *);
68int irplib_stdstar_select_stars_dist(cpl_table *, double, double, double);
69int irplib_stdstar_select_stars_mag(cpl_table *, const char *);
70int irplib_stdstar_find_closest(const cpl_table *, double, double);
71cpl_error_code irplib_stdstar_find_star(const char *, double, double, const char *,
72 const char *, double *, char **, char **, char **,
73 double *, double * , double);
74cpl_vector * irplib_stdstar_get_conversion(const cpl_bivector *, double, double,
75 double, double);
76cpl_vector * irplib_stdstar_get_mag_zero(const cpl_bivector *,
77 const cpl_vector *, double);
78cpl_bivector * irplib_stdstar_get_sed(const char *, const char *);
79
80#endif
int irplib_stdstar_select_stars_dist(cpl_table *, double, double, double)
Deselect the stars that are beyond a given distance.
int irplib_stdstar_select_stars_mag(cpl_table *, const char *)
Select the stars that have a known magnitude.
cpl_error_code irplib_stdstar_check_columns_exist(const cpl_table *)
Check that the table has the relevant columns of a stdstar table.
int irplib_stdstar_find_closest(const cpl_table *, double, double)
Find the closest star.
cpl_error_code irplib_stdstar_find_star(const char *, double, double, const char *, const char *, double *, char **, char **, char **, double *, double *, double)
Find the closest star to ra, dec in the catalog.
cpl_table * irplib_stdstar_load_catalog(const char *, const char *)
Load the FITS catalog in a table.
cpl_vector * irplib_stdstar_get_conversion(const cpl_bivector *, double, double, double, double)
Get the conversion.
cpl_error_code irplib_stdstar_write_catalogs(cpl_frameset *set_in, const cpl_frameset *set_raw, const char *recipe_name, const char *pro_cat, const char *pro_type, const char *package_name, const char *ins_name, cpl_table *(*convert_ascii_table)(const char *))
Write the ASCII catalogs as FITS files.
cpl_vector * irplib_stdstar_get_mag_zero(const cpl_bivector *, const cpl_vector *, double)
Get the 0 magnitude spectrum.
cpl_bivector * irplib_stdstar_get_sed(const char *, const char *)
Get the SED.