LSST Applications g04e9c324dd+8c5ae1fdc5,g134cb467dc+b203dec576,g18429d2f64+358861cd2c,g199a45376c+0ba108daf9,g1fd858c14a+dd066899e3,g262e1987ae+ebfced1d55,g29ae962dfc+72fd90588e,g2cef7863aa+aef1011c0b,g35bb328faa+8c5ae1fdc5,g3fd5ace14f+b668f15bc5,g4595892280+3897dae354,g47891489e3+abcf9c3559,g4d44eb3520+fb4ddce128,g53246c7159+8c5ae1fdc5,g67b6fd64d1+abcf9c3559,g67fd3c3899+1f72b5a9f7,g74acd417e5+cb6b47f07b,g786e29fd12+668abc6043,g87389fa792+8856018cbb,g89139ef638+abcf9c3559,g8d7436a09f+bcf525d20c,g8ea07a8fe4+9f5ccc88ac,g90f42f885a+6054cc57f1,g97be763408+06f794da49,g9dd6db0277+1f72b5a9f7,ga681d05dcb+7e36ad54cd,gabf8522325+735880ea63,gac2eed3f23+abcf9c3559,gb89ab40317+abcf9c3559,gbf99507273+8c5ae1fdc5,gd8ff7fe66e+1f72b5a9f7,gdab6d2f7ff+cb6b47f07b,gdc713202bf+1f72b5a9f7,gdfd2d52018+8225f2b331,ge365c994fd+375fc21c71,ge410e46f29+abcf9c3559,geaed405ab2+562b3308c0,gf9a733ac38+8c5ae1fdc5,w.2025.35
LSST Data Management Base Package
Loading...
Searching...
No Matches
photometryTransform.cc
Go to the documentation of this file.
1// -*- LSST-C++ -*-
2/*
3 * This file is part of jointcal.
4 *
5 * Developed for the LSST Data Management System.
6 * This product includes software developed by the LSST Project
7 * (https://www.lsst.org).
8 * See the COPYRIGHT file at the top-level directory of this distribution
9 * for details of code ownership.
10 *
11 * This program is free software: you can redistribute it and/or modify
12 * it under the terms of the GNU General Public License as published by
13 * the Free Software Foundation, either version 3 of the License, or
14 * (at your option) any later version.
15 *
16 * This program is distributed in the hope that it will be useful,
17 * but WITHOUT ANY WARRANTY; without even the implied warranty of
18 * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
19 * GNU General Public License for more details.
20 *
21 * You should have received a copy of the GNU General Public License
22 * along with this program. If not, see <https://www.gnu.org/licenses/>.
23 */
24
25#include "pybind11/pybind11.h"
27#include "pybind11/eigen.h"
28#include "ndarray/pybind11.h"
29#include "ndarray/eigen.h"
30#include "Eigen/Core"
31
33
34namespace py = pybind11;
35using namespace pybind11::literals;
36
37namespace lsst {
38namespace jointcal {
39namespace {
40
41void declarePhotometryTransform(lsst::cpputils::python::WrapperCollection &wrappers) {
42 using PyPhotometryTransform = py::classh<PhotometryTransform>;
43
44 wrappers.wrapType(PyPhotometryTransform(wrappers.module, "PhotometryTransform"), [](auto &mod, auto &cls) {
45 cls.def("transform",
46 (double (PhotometryTransform::*)(double, double, double) const) &PhotometryTransform::transform,
47 "x"_a, "y"_a, "value"_a);
48 cls.def("transformError",
49 (double (PhotometryTransform::*)(double, double, double, double) const) &
50 PhotometryTransform::transformError,
51 "x"_a, "y"_a, "value"_a, "valueErr"_a);
52 cls.def("offsetParams", &PhotometryTransform::offsetParams);
53 cls.def("clone", &PhotometryTransform::clone);
54 cls.def("getNpar", &PhotometryTransform::getNpar);
55 cls.def("getParameters", &PhotometryTransform::getParameters);
56 cls.def("computeParameterDerivatives",
57 [](PhotometryTransform const &self, double x, double y, double instFlux) {
58 Eigen::VectorXd derivatives(self.getNpar());
59 self.computeParameterDerivatives(x, y, instFlux, derivatives);
60 return derivatives;
61 });
62 cpputils::python::addOutputOp(cls, "__str__");
63 cpputils::python::addOutputOp(cls, "__repr__");
64 });
65}
66
67void declarePhotometryTransformSpatiallyInvariant(lsst::cpputils::python::WrapperCollection &wrappers) {
68 using PyPhotometryTransformSpatiallyInvariant = py::classh<PhotometryTransformSpatiallyInvariant,
70
71 wrappers.wrapType(
72 PyPhotometryTransformSpatiallyInvariant(
73 wrappers.module, "PhotometryTransformSpatiallyInvariant"), [](auto &mod, auto &cls) {});
74}
75
76void declareFluxTransformSpatiallyInvariant(lsst::cpputils::python::WrapperCollection &wrappers) {
77 using PyFluxTransformSpatiallyInvariant = py::classh<FluxTransformSpatiallyInvariant,
79
80 wrappers.wrapType(
81 PyFluxTransformSpatiallyInvariant(
82 wrappers.module, "FluxTransformSpatiallyInvariant"), [](auto &mod, auto &cls) {
83 cls.def(py::init<double>(), "value"_a = 1);
84 });
85}
86
87void declareMagnitudeTransformSpatiallyInvariant(lsst::cpputils::python::WrapperCollection &wrappers) {
88 using PyMagnitudeTransformSpatiallyInvariant = py::classh<MagnitudeTransformSpatiallyInvariant,
90
91 wrappers.wrapType(
92 PyMagnitudeTransformSpatiallyInvariant(
93 wrappers.module, "MagnitudeTransformSpatiallyInvariant"), [](auto &mod, auto &cls) {
94 cls.def(py::init<double>(), "value"_a = 0);
95 });
96}
97
98void declarePhotometryTransformChebyshev(lsst::cpputils::python::WrapperCollection &wrappers) {
99 using PyPhotometryTransformChebyshev =
100 py::classh<PhotometryTransformChebyshev, PhotometryTransform>;
101
102 wrappers.wrapType(PyPhotometryTransformChebyshev(
103 wrappers.module, "PhotometryTransformChebyshev"), [](auto &mod, auto &cls) {
104 cls.def("getCoefficients", &PhotometryTransformChebyshev::getCoefficients);
105 cls.def("getOrder", &PhotometryTransformChebyshev::getOrder);
106 cls.def("getBBox", &PhotometryTransformChebyshev::getBBox);
107 cls.def("integrate", py::overload_cast<>(&PhotometryTransformChebyshev::integrate, py::const_));
108 cls.def("integrate",
109 py::overload_cast<geom::Box2D const &>(&PhotometryTransformChebyshev::integrate, py::const_),
110 "box"_a);
111 });
112}
113
114void declareFluxTransformChebyshev(lsst::cpputils::python::WrapperCollection &wrappers) {
115 using PyFluxTransformChebyshev =
116 py::classh<FluxTransformChebyshev, PhotometryTransformChebyshev>;
117
118 wrappers.wrapType(PyFluxTransformChebyshev(wrappers.module, "FluxTransformChebyshev"), [](auto &mod, auto &cls) {
119 cls.def(py::init<size_t, geom::Box2D const &>(), "order"_a, "bbox"_a);
120 cls.def(py::init<ndarray::Array<double, 2, 2> const &, geom::Box2D const &>(), "coefficients"_a,
121 "bbox"_a);
122 });
123}
124
125void declareMagnitudeTransformChebyshev(lsst::cpputils::python::WrapperCollection &wrappers) {
126 using PyMagnitudeTransformChebyshev = py::classh<MagnitudeTransformChebyshev,
128
129 wrappers.wrapType(
130 PyMagnitudeTransformChebyshev(wrappers.module, "MagnitudeTransformChebyshev"), [](auto &mod, auto &cls) {
131 cls.def(py::init<size_t, geom::Box2D const &>(), "order"_a, "bbox"_a);
132 cls.def(py::init<ndarray::Array<double, 2, 2> const &, geom::Box2D const &>(), "coefficients"_a,
133 "bbox"_a);
134 });
135}
136} // namespace
137
139 declarePhotometryTransform(wrappers);
140 declarePhotometryTransformSpatiallyInvariant(wrappers);
141 declareFluxTransformSpatiallyInvariant(wrappers);
142 declareMagnitudeTransformSpatiallyInvariant(wrappers);
143 declarePhotometryTransformChebyshev(wrappers);
144 declareFluxTransformChebyshev(wrappers);
145 declareMagnitudeTransformChebyshev(wrappers);
146}
147
148} // namespace jointcal
149} // namespace lsst
A helper class for subdividing pybind11 module across multiple translation units (i....
Definition python.h:242
PyType wrapType(PyType cls, ClassWrapperCallback function, bool setModuleName=true)
Add a type (class or enum) wrapper, deferring method and other attribute definitions until finish() i...
Definition python.h:391
pybind11::module module
The module object passed to the PYBIND11_MODULE block that contains this WrapperCollection.
Definition python.h:448
Photometric offset independent of position, defined as (fluxMag0)^-1.
nth-order 2d Chebyshev photometry transform, plus the input flux.
Photometric offset independent of position, defined as -2.5 * log(flux / fluxMag0).
nth-order 2d Chebyshev photometry transform.
A photometric transform, defined in terms of the input flux or magnitude.
Photometry offset independent of position.
void addOutputOp(PyClass &cls, std::string const &method)
Add __str__ or __repr__ method implemented by operator<<.
Definition python.h:87
void wrapPhotometryTransform(WrapperCollection &wrappers)