LSSTApplications  11.0-13-gbb96280,12.1+18,12.1+7,12.1-1-g14f38d3+72,12.1-1-g16c0db7+5,12.1-1-g5961e7a+84,12.1-1-ge22e12b+23,12.1-11-g06625e2+4,12.1-11-g0d7f63b+4,12.1-19-gd507bfc,12.1-2-g7dda0ab+38,12.1-2-gc0bc6ab+81,12.1-21-g6ffe579+2,12.1-21-gbdb6c2a+4,12.1-24-g941c398+5,12.1-3-g57f6835+7,12.1-3-gf0736f3,12.1-37-g3ddd237,12.1-4-gf46015e+5,12.1-5-g06c326c+20,12.1-5-g648ee80+3,12.1-5-gc2189d7+4,12.1-6-ga608fc0+1,12.1-7-g3349e2a+5,12.1-7-gfd75620+9,12.1-9-g577b946+5,12.1-9-gc4df26a+10
LSSTDataManagementBasePackage
Namespaces | Functions
PeakLikelihoodFlux.cc File Reference
#include "ndarray/eigen.h"
#include "lsst/afw/detection/Psf.h"
#include "lsst/afw/geom/Box.h"
#include "lsst/pex/exceptions.h"
#include "lsst/afw/geom.h"
#include "lsst/afw/image.h"
#include "lsst/afw/math.h"
#include "lsst/meas/base/PeakLikelihoodFlux.h"
#include "lsst/afw/table/Source.h"

Go to the source code of this file.

Namespaces

 lsst
 Remove all non-astronomical counts from the Chunk Exposure's pixels.
 
 lsst::meas
 
 lsst::meas::base
 

Functions

template<typename T >
afw::image::MaskedImage< T >
::SinglePixel 
lsst::meas::base::computeShiftedValue (afw::image::MaskedImage< T > const &maskedImage, std::string const &warpingKernelName, afw::geom::Point2D const &fracShift, afw::geom::Point2I const &parentInd)
 Compute the value of one pixel of an image after a fractional pixel shift Since we only want the value at one pixel, there is no need to shift the entire image; instead we simply convolve at one point. More...
 

Variable Documentation

boost::shared_ptr< lsst::afw::image::Image<double> > _psfImage

Definition at line 73 of file PeakLikelihoodFlux.cc.