LSST Applications
21.0.0-172-gfb10e10a+18fedfabac,22.0.0+297cba6710,22.0.0+80564b0ff1,22.0.0+8d77f4f51a,22.0.0+a28f4c53b1,22.0.0+dcf3732eb2,22.0.1-1-g7d6de66+2a20fdde0d,22.0.1-1-g8e32f31+297cba6710,22.0.1-1-geca5380+7fa3b7d9b6,22.0.1-12-g44dc1dc+2a20fdde0d,22.0.1-15-g6a90155+515f58c32b,22.0.1-16-g9282f48+790f5f2caa,22.0.1-2-g92698f7+dcf3732eb2,22.0.1-2-ga9b0f51+7fa3b7d9b6,22.0.1-2-gd1925c9+bf4f0e694f,22.0.1-24-g1ad7a390+a9625a72a8,22.0.1-25-g5bf6245+3ad8ecd50b,22.0.1-25-gb120d7b+8b5510f75f,22.0.1-27-g97737f7+2a20fdde0d,22.0.1-32-gf62ce7b1+aa4237961e,22.0.1-4-g0b3f228+2a20fdde0d,22.0.1-4-g243d05b+871c1b8305,22.0.1-4-g3a563be+32dcf1063f,22.0.1-4-g44f2e3d+9e4ab0f4fa,22.0.1-42-gca6935d93+ba5e5ca3eb,22.0.1-5-g15c806e+85460ae5f3,22.0.1-5-g58711c4+611d128589,22.0.1-5-g75bb458+99c117b92f,22.0.1-6-g1c63a23+7fa3b7d9b6,22.0.1-6-g50866e6+84ff5a128b,22.0.1-6-g8d3140d+720564cf76,22.0.1-6-gd805d02+cc5644f571,22.0.1-8-ge5750ce+85460ae5f3,master-g6e05de7fdc+babf819c66,master-g99da0e417a+8d77f4f51a,w.2021.48
LSST Data Management Base Package
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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 |