File SimpleAstrometryModel.h¶
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namespace
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
- Note
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.
- Note
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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namespace
jointcal -
class
SimpleAstrometryModel: public lsst::jointcal::AstrometryModel - #include <SimpleAstrometryModel.h>
A model where there is one independent transform per CcdImage.
This modeling of distortions can even accommodate images set mixing instruments
- Parameters
ccdImageList: The exposures that will be fit.projectionHandler: The projection from “Sky” (where the “true” coordinates live) to “Tangent Plane” (where the fitting occurs).initFromWCS: Initialize the model parameters from the original exposure Wcs parameters?nNotFit: How many exposure to hold fixed and not be fit? (the first n will be selected) .order: The polynomial order of each exposure’s pixel-tangent plane mapping.
Public Functions
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SimpleAstrometryModel(SimpleAstrometryModel const&) No copy or move: there is only ever one instance of a given model (i.e.. per ccd+visit)
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SimpleAstrometryModel(SimpleAstrometryModel&&)
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SimpleAstrometryModel &
operator=(SimpleAstrometryModel const&)
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SimpleAstrometryModel &
operator=(SimpleAstrometryModel&&)
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const AstrometryMapping *
getMapping(CcdImage const&) const Mapping associated to a given CcdImage.
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Eigen::Index
assignIndices(std::string const &whatToFit, Eigen::Index firstIndex) Positions the various parameter sets into the parameter vector, starting at firstIndex.
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void
offsetParams(Eigen::VectorXd const &delta) Offset the parameters by the provided amounts (by -delta).
The shifts are applied according to the indices given in assignIndices.
- Parameters
[in] delta: vector of offsets to apply
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const std::shared_ptr<AstrometryTransform const>
getSkyToTangentPlane(CcdImage const &ccdImage) const the mapping of sky coordinates (i.e. the coordinate system in which fitted stars are reported) onto the Tangent plane (into which the pixel coordinates are transformed)
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void
freezeErrorTransform()
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std::size_t
getTotalParameters() const Return the total number of parameters in this model.
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AstrometryTransform const &
getTransform(CcdImage const &ccdImage) const Access to mappings.
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std::shared_ptr<afw::geom::SkyWcs>
makeSkyWcs(CcdImage const &ccdImage) const Make a SkyWcs that contains this model.
- Return
SkyWcs containing this model.
- Parameters
ccdImage: The exposure to create the SkyWcs for.
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~SimpleAstrometryModel()
Private Functions
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AstrometryMapping *
findMapping(CcdImage const &ccdImage) const¶ Return a pointer to the mapping associated with this ccdImage.
Private Members
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std::unordered_map<CcdImageKey, std::unique_ptr<SimpleAstrometryMapping>>
_myMap¶
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const std::shared_ptr<ProjectionHandler const>
_skyToTangentPlane¶
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class