25#include "pybind11/pybind11.h"
26#include "pybind11/eigen.h"
27#include "pybind11/stl.h"
28#include "ndarray/pybind11.h"
29#include "ndarray/eigen.h"
41using namespace pybind11::literals;
48 py::class_<PhotometryModel, std::shared_ptr<PhotometryModel>> cls(mod,
"PhotometryModel");
67 cls.def(
"computeParameterDerivatives",
68 [](PhotometryModel
const &
self, MeasuredStar
const &star, CcdImage
const &ccdImage) {
69 Eigen::VectorXd derivatives(
self.getNpar(ccdImage));
70 self.computeParameterDerivatives(star, ccdImage, derivatives);
80 cls.def(
"__str__", [](PhotometryModel
const &
self) {
return "PhotometryModel"; });
83void declareSimplePhotometryModel(
py::module &mod) {
84 py::class_<SimplePhotometryModel, std::shared_ptr<SimplePhotometryModel>, PhotometryModel> cls(
85 mod,
"SimplePhotometryModel");
86 cls.def(
"__str__", [](SimplePhotometryModel
const &
self) {
return "SimplePhotometryModel"; });
90 py::class_<SimpleFluxModel, std::shared_ptr<SimpleFluxModel>, SimplePhotometryModel, PhotometryModel> cls(
91 mod,
"SimpleFluxModel");
92 cls.def(py::init<CcdImageList const &, double>(),
"ccdImageList"_a,
"errorPedestal"_a = 0);
94 cls.def(
"__str__", [](SimpleFluxModel
const &
self) {
return "SimpleFluxModel"; });
97void declareSimpleMagnitudeModel(
py::module &mod) {
98 py::class_<SimpleMagnitudeModel, std::shared_ptr<SimpleMagnitudeModel>, SimplePhotometryModel,
100 cls(mod,
"SimpleMagnitudeModel");
101 cls.def(py::init<CcdImageList const &, double>(),
"ccdImageList"_a,
"errorPedestal"_a = 0);
103 cls.def(
"__str__", [](SimpleMagnitudeModel
const &
self) {
return "SimpleMagnitudeModel"; });
106void declareConstrainedPhotometryModel(
py::module &mod) {
107 py::class_<ConstrainedPhotometryModel, std::shared_ptr<ConstrainedPhotometryModel>, PhotometryModel> cls(
108 mod,
"ConstrainedPhotometryModel");
109 cls.def(
"__str__", [](ConstrainedPhotometryModel
const &
self) {
return "ConstrainedPhotometryModel"; });
112void declareConstrainedFluxModel(
py::module &mod) {
113 py::class_<ConstrainedFluxModel, std::shared_ptr<ConstrainedFluxModel>, PhotometryModel> cls(
114 mod,
"ConstrainedFluxModel");
115 cls.def(py::init<CcdImageList const &, lsst::geom::Box2D const &, int, double>(),
"CcdImageList"_a,
116 "bbox"_a,
"visitOrder"_a = 7,
"errorPedestal"_a = 0);
117 cls.def(
"__str__", [](ConstrainedFluxModel
const &
self) {
return "ConstrainedFluxModel"; });
120void declareConstrainedMagnitudeModel(
py::module &mod) {
121 py::class_<ConstrainedMagnitudeModel, std::shared_ptr<ConstrainedMagnitudeModel>, PhotometryModel> cls(
122 mod,
"ConstrainedMagnitudeModel");
123 cls.def(py::init<CcdImageList const &, lsst::geom::Box2D const &, int, double>(),
"CcdImageList"_a,
124 "bbox"_a,
"visitOrder"_a = 7,
"errorPedestal"_a = 0);
125 cls.def(
"__str__", [](ConstrainedMagnitudeModel
const &
self) {
return "ConstrainedMagnitudeModel"; });
129 py::module::import(
"lsst.jointcal.ccdImage");
130 py::module::import(
"lsst.jointcal.photometryTransform");
131 py::module::import(
"lsst.jointcal.star");
132 declarePhotometryModel(mod);
133 declareSimplePhotometryModel(mod);
134 declareSimpleFluxModel(mod);
135 declareSimpleMagnitudeModel(mod);
136 declareConstrainedPhotometryModel(mod);
137 declareConstrainedFluxModel(mod);
138 declareConstrainedMagnitudeModel(mod);
virtual std::size_t getTotalParameters() const =0
Return the total number of parameters in this model.
virtual Eigen::Index assignIndices(std::string const &whatToFit, Eigen::Index firstIndex)=0
Assign indices in the full matrix to the parameters being fit in the mappings, starting at firstIndex...
virtual void offsetParams(Eigen::VectorXd const &delta)=0
Offset the parameters by the provided amounts (by -delta).
virtual double transform(CcdImage const &ccdImage, MeasuredStar const &measuredStar) const =0
Return the on-sky transformed flux for measuredStar on ccdImage.
virtual double getRefError(RefStar const &refStar) const =0
Return the refStar error appropriate for this model (e.g. fluxErr or magErr).
bool validate(CcdImageList const &ccdImageList, int ndof) const
Return true if this is a "reasonable" model.
PhotometryMappingBase const & getMapping(CcdImage const &ccdImage) const
Get the mapping associated with ccdImage.
virtual void offsetFittedStar(FittedStar &fittedStar, double delta) const =0
Offset the appropriate flux or magnitude (by -delta).
virtual void freezeErrorTransform()=0
Once this routine has been called, the error transform is not modified by offsetParams().
virtual double computeResidual(CcdImage const &ccdImage, MeasuredStar const &measuredStar) const =0
Compute the residual between the model applied to a star and its associated fittedStar.
std::size_t getNpar(CcdImage const &ccdImage) const
Return the number of parameters in the mapping of CcdImage.
virtual void getMappingIndices(CcdImage const &ccdImage, IndexVector &indices) const =0
Get how this set of parameters (of length Npar()) map into the "grand" fit.
virtual std::shared_ptr< afw::image::PhotoCalib > toPhotoCalib(CcdImage const &ccdImage) const =0
Return the mapping of ccdImage represented as a PhotoCalib.
bool checkPositiveOnBBox(CcdImage const &ccdImage) const
Check that the model is positive on the ccdImage bbox.
virtual double computeRefResidual(FittedStar const &fittedStar, RefStar const &refStar) const =0
Return the fittedStar - refStar residual appropriate for this model (e.g. flux - flux or mag - mag).
virtual double transformError(CcdImage const &ccdImage, MeasuredStar const &measuredStar) const =0
Return the on-sky transformed flux uncertainty for measuredStar on ccdImage.
PYBIND11_MODULE(_cameraGeom, mod)
void addOutputOp(PyClass &cls, std::string const &method)
Add __str__ or __repr__ method implemented by operator<<.
A base class for image defects.