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LSSTApplications
20.0.0
LSSTDataManagementBasePackage
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Detect cosmic rays in a MaskedImage. More...
#include <stdexcept>#include <algorithm>#include <cassert>#include <string>#include <typeinfo>#include <iostream>#include "boost/format.hpp"#include "lsst/pex/exceptions.h"#include "lsst/log/Log.h"#include "lsst/afw/detection/Footprint.h"#include "lsst/afw/geom.h"#include "lsst/afw/detection/Psf.h"#include "lsst/afw/image/MaskedImage.h"#include "lsst/afw/math/Random.h"#include "lsst/meas/algorithms/CR.h"#include "lsst/meas/algorithms/Interp.h"Go to the source code of this file.
Classes | |
| class | lsst::afw::detection::IdSpan |
| run-length code for part of object More... | |
| struct | lsst::afw::detection::IdSpanCompar |
| comparison functor; sort by ID, then by row (y), then by column range start (x0) More... | |
Namespaces | |
| lsst | |
| A base class for image defects. | |
| lsst::afw | |
| lsst::afw::detection | |
| lsst::meas | |
| lsst::meas::algorithms | |
| Fit spatial kernel using approximate fluxes for candidates, and solving a linear system of equations. | |
Functions | |
| int | lsst::afw::detection::resolve_alias (const std::vector< int > &aliases, int id) |
| Follow a chain of aliases, returning the final resolved value. More... | |
| template<typename MaskedImageT > | |
| std::vector< std::shared_ptr< afw::detection::Footprint > > | lsst::meas::algorithms::findCosmicRays (MaskedImageT &mimage, afw::detection::Psf const &psf, double const bkgd, daf::base::PropertySet const &ps, bool const keep) |
| Find cosmic rays in an Image, and mask and remove them. More... | |
Detect cosmic rays in a MaskedImage.
Definition in file CR.cc.
| ImageT val |
1.8.18