LSSTApplications
10.0+286,10.0+36,10.0+46,10.0-2-g4f67435,10.1+152,10.1+37,11.0,11.0+1,11.0-1-g47edd16,11.0-1-g60db491,11.0-1-g7418c06,11.0-2-g04d2804,11.0-2-g68503cd,11.0-2-g818369d,11.0-2-gb8b8ce7
LSSTDataManagementBasePackage
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C++ control object for peak likelihood flux. More...
#include <PeakLikelihoodFlux.h>
Public Member Functions | |
PeakLikelihoodFluxControl () | |
Public Attributes | |
std::string | warpingKernelName |
"Name of warping kernel (e.g. \"lanczos4") used to compute the peak" ; More... | |
C++ control object for peak likelihood flux.
Peak likelihood flux requires an image that has been filtered by convolving with its own PSF (or an approximate model). It is equivalent to a PSF flux (e.g. PsfFluxAlgorithm) computed on a non-preconvolved image.
The PSF must be provided in the exposure, as it is used to compute a weighting factor.
Flux and error are computed as follows:
Definition at line 57 of file PeakLikelihoodFlux.h.
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inline |
Definition at line 63 of file PeakLikelihoodFlux.h.
std::string lsst::meas::base::PeakLikelihoodFluxControl::warpingKernelName |
"Name of warping kernel (e.g. \"lanczos4") used to compute the peak" ;
Definition at line 61 of file PeakLikelihoodFlux.h.