MUSE Pipeline Reference Manual
2.1.1
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muse
muse_artifacts.h
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/* -*- Mode: C; tab-width: 2; indent-tabs-mode: nil; c-basic-offset: 2 -*- */
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/* vim:set sw=2 sts=2 et cin: */
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/*
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* This file is part of the MUSE Instrument Pipeline
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* Copyright (C) 2005-2014 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, Inc., 51 Franklin Street, Fifth Floor, Boston, MA 02110-1301, USA.
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*/
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#ifndef MUSE_ARTIFACTS_H
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#define MUSE_ARTIFACTS_H
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/*----------------------------------------------------------------------------*
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* Includes *
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*----------------------------------------------------------------------------*/
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#include <cpl.h>
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#include "muse_image.h"
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/*----------------------------------------------------------------------------*
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* Function prototypes *
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*----------------------------------------------------------------------------*/
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int
muse_cosmics_dcr
(
muse_image
*,
unsigned
int
,
unsigned
int
,
unsigned
int
,
float
);
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#endif
/* MUSE_ARTIFACTS_H */
muse_cosmics_dcr
int muse_cosmics_dcr(muse_image *, unsigned int, unsigned int, unsigned int, float)
Quickly mark cosmic rays in an image using the DCR algorithm.
Definition:
muse_artifacts.c:275
muse_image
Structure definition of MUSE three extension FITS file.
Definition:
muse_image.h:40
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