CR.h

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// -*- LSST-C++ -*-

/*
 * LSST Data Management System
 * Copyright 2008, 2009, 2010 LSST Corporation.
 *
 * This product includes software developed by the
 * LSST Project (http://www.lsst.org/).
 *
 * 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 3 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 LSST License Statement and
 * the GNU General Public License along with this program.  If not,
 * see <http://www.lsstcorp.org/LegalNotices/>.
 */

#if !defined(LSST_MEAS_ALGORITHMS_CR_H)
#define LSST_MEAS_ALGORITHMS_CR_H
// Handle cosmic rays in a MaskedImage
//
#include <vector>
#include "lsst/base.h"
#include "lsst/daf/base.h"
#include "lsst/afw/image/MaskedImage.h"

namespace lsst {
namespace afw {
namespace detection {
class Footprint;
class Psf;
}  // namespace detection
}  // namespace afw
}  // namespace lsst

namespace lsst {
namespace meas {
namespace algorithms {

template <typename MaskedImageT>
std::vector<std::shared_ptr<afw::detection::Footprint> > findCosmicRays(MaskedImageT& image,
                                                                        afw::detection::Psf const& psf,
                                                                        double const bkgd,
                                                                        daf::base::PropertySet const& ps,
                                                                        bool const keep = false);
}
}  // namespace meas
}  // namespace lsst

#endif