LSSTApplications  17.0+11,17.0+34,17.0+56,17.0+57,17.0+59,17.0+7,17.0-1-g377950a+33,17.0.1-1-g114240f+2,17.0.1-1-g4d4fbc4+28,17.0.1-1-g55520dc+49,17.0.1-1-g5f4ed7e+52,17.0.1-1-g6dd7d69+17,17.0.1-1-g8de6c91+11,17.0.1-1-gb9095d2+7,17.0.1-1-ge9fec5e+5,17.0.1-1-gf4e0155+55,17.0.1-1-gfc65f5f+50,17.0.1-1-gfc6fb1f+20,17.0.1-10-g87f9f3f+1,17.0.1-11-ge9de802+16,17.0.1-16-ga14f7d5c+4,17.0.1-17-gc79d625+1,17.0.1-17-gdae4c4a+8,17.0.1-2-g26618f5+29,17.0.1-2-g54f2ebc+9,17.0.1-2-gf403422+1,17.0.1-20-g2ca2f74+6,17.0.1-23-gf3eadeb7+1,17.0.1-3-g7e86b59+39,17.0.1-3-gb5ca14a,17.0.1-3-gd08d533+40,17.0.1-30-g596af8797,17.0.1-4-g59d126d+4,17.0.1-4-gc69c472+5,17.0.1-6-g5afd9b9+4,17.0.1-7-g35889ee+1,17.0.1-7-gc7c8782+18,17.0.1-9-gc4bbfb2+3,w.2019.22
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
9  * it under the terms of the GNU General Public License as published by
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12  *
13  * This program is distributed in the hope that it will be useful,
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16  * GNU General Public License for more details.
17  *
18  * You should have received a copy of the LSST License Statement and
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20  * see <https://www.lsstcorp.org/LegalNotices/>.
21  */
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 
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 
PYBIND11_MODULE(baselineUtils, mod)
py::object result
Definition: schema.cc:418
A set of pixels in an Image, including those pixels&#39; actual values.
STL class.
A base class for image defects.
A class to manipulate images, masks, and variance as a single object.
Definition: MaskedImage.h:74
std::int32_t MaskPixel
default type for Masks and MaskedImage Masks
Class to describe the properties of a detected object from an image.
Definition: Footprint.h:62
STL class.
def apportionFlux(debResult, log, assignStrayFlux=True, strayFluxAssignment='r-to-peak', strayFluxToPointSources='necessary', clipStrayFluxFraction=0.001, getTemplateSum=False)
Definition: plugins.py:1398
float VariancePixel
default type for MaskedImage variance images
Record class that represents a peak in a Footprint.
Definition: Peak.h:42
A class to represent a 2-dimensional array of pixels.
Definition: Image.h:59
table::Key< double > sigma1