MUSE Pipeline Reference Manual  2.1.1
muse_artifacts.h
1 /* -*- Mode: C; tab-width: 2; indent-tabs-mode: nil; c-basic-offset: 2 -*- */
2 /* vim:set sw=2 sts=2 et cin: */
3 /*
4  * This file is part of the MUSE Instrument Pipeline
5  * Copyright (C) 2005-2014 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
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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.
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20  */
21 
22 #ifndef MUSE_ARTIFACTS_H
23 #define MUSE_ARTIFACTS_H
24 
25 /*----------------------------------------------------------------------------*
26  * Includes *
27  *----------------------------------------------------------------------------*/
28 #include <cpl.h>
29 
30 #include "muse_image.h"
31 
32 /*----------------------------------------------------------------------------*
33  * Function prototypes *
34  *----------------------------------------------------------------------------*/
35 int muse_cosmics_dcr(muse_image *, unsigned int, unsigned int, unsigned int, float);
36 
37 #endif /* MUSE_ARTIFACTS_H */
int muse_cosmics_dcr(muse_image *, unsigned int, unsigned int, unsigned int, float)
Quickly mark cosmic rays in an image using the DCR algorithm.
Structure definition of MUSE three extension FITS file.
Definition: muse_image.h:40