LSST Applications
21.0.0-147-g0e635eb1+1acddb5be5,22.0.0+052faf71bd,22.0.0+1ea9a8b2b2,22.0.0+6312710a6c,22.0.0+729191ecac,22.0.0+7589c3a021,22.0.0+9f079a9461,22.0.1-1-g7d6de66+b8044ec9de,22.0.1-1-g87000a6+536b1ee016,22.0.1-1-g8e32f31+6312710a6c,22.0.1-10-gd060f87+016f7cdc03,22.0.1-12-g9c3108e+df145f6f68,22.0.1-16-g314fa6d+c825727ab8,22.0.1-19-g93a5c75+d23f2fb6d8,22.0.1-19-gb93eaa13+aab3ef7709,22.0.1-2-g8ef0a89+b8044ec9de,22.0.1-2-g92698f7+9f079a9461,22.0.1-2-ga9b0f51+052faf71bd,22.0.1-2-gac51dbf+052faf71bd,22.0.1-2-gb66926d+6312710a6c,22.0.1-2-gcb770ba+09e3807989,22.0.1-20-g32debb5+b8044ec9de,22.0.1-23-gc2439a9a+fb0756638e,22.0.1-3-g496fd5d+09117f784f,22.0.1-3-g59f966b+1e6ba2c031,22.0.1-3-g849a1b8+f8b568069f,22.0.1-3-gaaec9c0+c5c846a8b1,22.0.1-32-g5ddfab5d3+60ce4897b0,22.0.1-4-g037fbe1+64e601228d,22.0.1-4-g8623105+b8044ec9de,22.0.1-5-g096abc9+d18c45d440,22.0.1-5-g15c806e+57f5c03693,22.0.1-7-gba73697+57f5c03693,master-g6e05de7fdc+c1283a92b8,master-g72cdda8301+729191ecac,w.2021.39
LSST Data Management Base Package
|
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 |