LSSTApplications
19.0.0-14-gb0260a2+72efe9b372,20.0.0+7927753e06,20.0.0+8829bf0056,20.0.0+995114c5d2,20.0.0+b6f4b2abd1,20.0.0+bddc4f4cbe,20.0.0-1-g253301a+8829bf0056,20.0.0-1-g2b7511a+0d71a2d77f,20.0.0-1-g5b95a8c+7461dd0434,20.0.0-12-g321c96ea+23efe4bbff,20.0.0-16-gfab17e72e+fdf35455f6,20.0.0-2-g0070d88+ba3ffc8f0b,20.0.0-2-g4dae9ad+ee58a624b3,20.0.0-2-g61b8584+5d3db074ba,20.0.0-2-gb780d76+d529cf1a41,20.0.0-2-ged6426c+226a441f5f,20.0.0-2-gf072044+8829bf0056,20.0.0-2-gf1f7952+ee58a624b3,20.0.0-20-geae50cf+e37fec0aee,20.0.0-25-g3dcad98+544a109665,20.0.0-25-g5eafb0f+ee58a624b3,20.0.0-27-g64178ef+f1f297b00a,20.0.0-3-g4cc78c6+e0676b0dc8,20.0.0-3-g8f21e14+4fd2c12c9a,20.0.0-3-gbd60e8c+187b78b4b8,20.0.0-3-gbecbe05+48431fa087,20.0.0-38-ge4adf513+a12e1f8e37,20.0.0-4-g97dc21a+544a109665,20.0.0-4-gb4befbc+087873070b,20.0.0-4-gf910f65+5d3db074ba,20.0.0-5-gdfe0fee+199202a608,20.0.0-5-gfbfe500+d529cf1a41,20.0.0-6-g64f541c+d529cf1a41,20.0.0-6-g9a5b7a1+a1cd37312e,20.0.0-68-ga3f3dda+5fca18c6a4,20.0.0-9-g4aef684+e18322736b,w.2020.45
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 |