File ImagePsf.h¶
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lsst Class for a simple mapping implementing a generic AstrometryTransform.
Remove all non-astronomical counts from the Chunk Exposure’s pixels.
Forward declarations for lsst::utils::Cache
For details on the Cache class, see the Cache.h file.
It uses a template rather than a pointer so that the derived classes can use the specifics of the transform. The class simplePolyMapping overloads a few routines.
A base class for image defects
Numeric constants used by the Integrate.h integrator routines.
Compute Image Statistics
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Gauss-Kronrod-Patterson quadrature coefficients for use in quadpack routine qng. These coefficients were calculated with 101 decimal digit arithmetic by L. W. Fullerton, Bell Labs, Nov 1981.
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The Statistics class itself can only handle lsst::afw::image::MaskedImage() types. The philosophy has been to handle other types by making them look like lsst::afw::image::MaskedImage() and reusing that code. Users should have no need to instantiate a Statistics object directly, but should use the overloaded makeStatistics() factory functions.
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ImagePsf: public lsst::afw::table::io::PersistableFacade<ImagePsf>, public lsst::afw::detection::Psf - #include <ImagePsf.h>
An intermediate base class for Psfs that use an image representation.
ImagePsf exists only to provide implementations of doComputeApertureFlux and doComputeShape for its derived classes. These implementations use the SincFlux and SdssShape algorithms defined in meas_algorithms, and hence could not be included with the Psf base class in afw.
Subclassed by lsst::meas::algorithms::CoaddPsf, lsst::meas::algorithms::KernelPsf, lsst::meas::algorithms::WarpedPsf, lsst::meas::extensions::psfex::PsfexPsf
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