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LSST Data Management Base Package
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C++ control object for peak likelihood instrument 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" ; | |
C++ control object for peak likelihood instrument 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 instrument flux (e.g. as computed by 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 59 of file PeakLikelihoodFlux.h.
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inline |
Definition at line 64 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 62 of file PeakLikelihoodFlux.h.