LSSTApplications  21.0.0+75b29a8a7f,21.0.0+e70536a077,21.0.0-1-ga51b5d4+62c747d40b,21.0.0-11-ga6ea59e8e+47cba9fc36,21.0.0-2-g103fe59+914993bf7c,21.0.0-2-g1367e85+e2614ded12,21.0.0-2-g45278ab+e70536a077,21.0.0-2-g4bc9b9f+7b2b5f8678,21.0.0-2-g5242d73+e2614ded12,21.0.0-2-g54e2caa+6403186824,21.0.0-2-g7f82c8f+3ac4acbffc,21.0.0-2-g8dde007+04a6aea1af,21.0.0-2-g8f08a60+9402881886,21.0.0-2-ga326454+3ac4acbffc,21.0.0-2-ga63a54e+81dd751046,21.0.0-2-gc738bc1+5f65c6e7a9,21.0.0-2-gde069b7+26c92b3210,21.0.0-2-gecfae73+0993ddc9bd,21.0.0-2-gfc62afb+e2614ded12,21.0.0-21-gba890a8+5a4f502a26,21.0.0-23-g9966ff26+03098d1af8,21.0.0-3-g357aad2+8ad216c477,21.0.0-3-g4be5c26+e2614ded12,21.0.0-3-g6d51c4a+4d2fe0280d,21.0.0-3-g7d9da8d+75b29a8a7f,21.0.0-3-gaa929c8+522e0f12c2,21.0.0-3-ge02ed75+4d2fe0280d,21.0.0-4-g3300ddd+e70536a077,21.0.0-4-gc004bbf+eac6615e82,21.0.0-4-gccdca77+f94adcd104,21.0.0-4-gd1c1571+18b81799f9,21.0.0-5-g7b47fff+4d2fe0280d,21.0.0-5-gb155db7+d2632f662b,21.0.0-5-gdf36809+637e4641ee,21.0.0-6-g722ad07+28c848f42a,21.0.0-7-g959bb79+522e0f12c2,21.0.0-7-gfd72ab2+cf01990774,21.0.0-9-g87fb7b8d+e2ab11cdd6,w.2021.04
LSSTDataManagementBasePackage
baselineUtils.cc
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1 /*
2  * LSST Data Management System
3  *
4  * This product includes software developed by the
5  * LSST Project (http://www.lsst.org/).
6  * See the COPYRIGHT file
7  *
8  * This program is free software: you can redistribute it and/or modify
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22 #include "pybind11/pybind11.h"
23 #include "pybind11/stl.h"
24 
25 #include "lsst/afw/image/Image.h"
29 
31 
32 namespace py = pybind11;
33 using namespace pybind11::literals;
34 
35 namespace lsst {
36 namespace meas {
37 namespace deblender {
38 
39 namespace {
40 
41 template <typename ImagePixelT, typename MaskPixelT = lsst::afw::image::MaskPixel,
42  typename VariancePixelT = lsst::afw::image::VariancePixel>
43 void declareBaselineUtils(py::module& mod, const std::string& suffix) {
47  using Class = BaselineUtils<ImagePixelT, MaskPixelT, VariancePixelT>;
48 
49  py::class_<Class, std::shared_ptr<Class>> cls(mod, ("BaselineUtils" + suffix).c_str());
50  cls.def_static("symmetrizeFootprint", &Class::symmetrizeFootprint, "foot"_a, "cx"_a, "cy"_a);
51  // The C++ function returns a std::pair return value but also takes a referenced boolean
52  // (patchedEdges) that is modified by the function and used by the python API,
53  // so we wrap this in a lambda to combine the std::pair and patchedEdges in a tuple
54  // that is returned to python.
55  cls.def_static("buildSymmetricTemplate", [](MaskedImageT const& img,
57  lsst::afw::detection::PeakRecord const& pk, double sigma1,
58  bool minZero, bool patchEdges) {
59  bool patchedEdges;
61 
62  result = Class::buildSymmetricTemplate(img, foot, pk, sigma1, minZero, patchEdges, &patchedEdges);
63  return py::make_tuple(result.first, result.second, patchedEdges);
64  });
65  cls.def_static("medianFilter", &Class::medianFilter, "img"_a, "outimg"_a, "halfsize"_a);
66  cls.def_static("makeMonotonic", &Class::makeMonotonic, "img"_a, "pk"_a);
67  // apportionFlux expects an empty vector containing HeavyFootprint pointers that is modified
68  // in the function. But when a list is passed to pybind11 in place of the vector,
69  // the changes are not passed back to python. So instead we create the vector in this lambda and
70  // include it in the return value.
71  cls.def_static("apportionFlux", [](MaskedImageT const& img, lsst::afw::detection::Footprint const& foot,
73  templates,
75  templ_footprints,
76  ImagePtrT templ_sum, std::vector<bool> const& ispsf,
77  std::vector<int> const& pkx, std::vector<int> const& pky,
78  int strayFluxOptions, double clipStrayFluxFraction) {
79  using HeavyFootprintPtrList = std::vector<std::shared_ptr<
81 
83  result;
84  HeavyFootprintPtrList strays;
85  result = Class::apportionFlux(img, foot, templates, templ_footprints, templ_sum, ispsf, pkx, pky,
86  strays, strayFluxOptions, clipStrayFluxFraction);
87 
88  return py::make_tuple(result, strays);
89  });
90  cls.def_static("hasSignificantFluxAtEdge", &Class::hasSignificantFluxAtEdge, "img"_a, "sfoot"_a,
91  "thresh"_a);
92  cls.def_static("getSignificantEdgePixels", &Class::getSignificantEdgePixels, "img"_a, "sfoot"_a,
93  "thresh"_a);
94  // There appears to be an issue binding to a static const member of a templated type, so for now
95  // we just use the values constants
96  cls.attr("ASSIGN_STRAYFLUX") = py::cast(Class::ASSIGN_STRAYFLUX);
97  cls.attr("STRAYFLUX_TO_POINT_SOURCES_WHEN_NECESSARY") =
98  py::cast(Class::STRAYFLUX_TO_POINT_SOURCES_WHEN_NECESSARY);
99  cls.attr("STRAYFLUX_TO_POINT_SOURCES_ALWAYS") = py::cast(Class::STRAYFLUX_TO_POINT_SOURCES_ALWAYS);
100  cls.attr("STRAYFLUX_R_TO_FOOTPRINT") = py::cast(Class::STRAYFLUX_R_TO_FOOTPRINT);
101  cls.attr("STRAYFLUX_NEAREST_FOOTPRINT") = py::cast(Class::STRAYFLUX_NEAREST_FOOTPRINT);
102  cls.attr("STRAYFLUX_TRIM") = py::cast(Class::STRAYFLUX_TRIM);
103 };
104 
105 } // <anonymous>
106 
107 PYBIND11_MODULE(baselineUtils, mod) {
108  py::module::import("lsst.afw.image");
109  py::module::import("lsst.afw.detection");
110 
111  declareBaselineUtils<float>(mod, "F");
112 }
113 
114 } // deblender
115 } // meas
116 } // lsst
117 
std::string
STL class.
std::shared_ptr
STL class.
lsst::afw::detection::PeakRecord
Record class that represents a peak in a Footprint.
Definition: Peak.h:42
BaselineUtils.h
std::pair
MaskedImage.h
std::vector
STL class.
Image.h
lsst::afw::geom.transform.transformContinued.cls
cls
Definition: transformContinued.py:33
lsst::meas::deblender::PYBIND11_MODULE
PYBIND11_MODULE(baselineUtils, mod)
Definition: baselineUtils.cc:107
lsst::afw::image::MaskedImage
A class to manipulate images, masks, and variance as a single object.
Definition: MaskedImage.h:73
lsst::afw::detection::HeavyFootprint
A set of pixels in an Image, including those pixels' actual values.
Definition: HeavyFootprint.h:49
lsst::afw::image::VariancePixel
float VariancePixel
default type for MaskedImage variance images
Definition: LsstImageTypes.h:35
sigma1
table::Key< double > sigma1
Definition: FunctionLibrary.cc:20
Footprint.h
lsst::afw::image::MaskPixel
std::int32_t MaskPixel
default type for Masks and MaskedImage Masks
Definition: LsstImageTypes.h:34
result
py::object result
Definition: _schema.cc:429
lsst
A base class for image defects.
Definition: imageAlgorithm.dox:1
Peak.h
pybind11
Definition: _GenericMap.cc:40
lsst::meas::deblender.plugins.apportionFlux
def apportionFlux(debResult, log, assignStrayFlux=True, strayFluxAssignment='r-to-peak', strayFluxToPointSources='necessary', clipStrayFluxFraction=0.001, getTemplateSum=False)
Definition: plugins.py:1216
lsst::afw::detection::Footprint
Class to describe the properties of a detected object from an image.
Definition: Footprint.h:63
lsst::afw::image::Image< ImagePixelT >
lsst::meas::modelfit.psf.psfContinued.module
module
Definition: psfContinued.py:42