LSST Applications 30.0.7,g0e76e35be5+e8e946ae08,g19811a7679+138f7293ba,g199a45376c+5e234f8357,g1fd858c14a+2f48dbc4c4,g262e1987ae+fb36cac54d,g29ae962dfc+d9108a0941,g2c21b0017a+4f59a27f16,g31e44d4a5c+b0138be388,g33ac35c1f1+28b9f72785,g35bb328faa+b0138be388,g40c9b15c53+823ad735c1,g47891489e3+bcc48a0b46,g53246c7159+b0138be388,g64539dfbff+e8e946ae08,g67b6fd64d1+bcc48a0b46,g74acd417e5+422380537a,g76965917b2+a5ca99c4d9,g786e29fd12+796b79145d,g7aefaa3e3d+dc0c200193,g86b635cae8+734fe384f0,g87389fa792+d8b5378923,g89139ef638+bcc48a0b46,g8bbb235e95+3f4f7f9447,g8ea07a8fe4+78a4c88802,g9290983e33+ffdc83c6f7,g92c671f44c+e8e946ae08,gaa753fd333+03f406da14,gbf99507273+b0138be388,gc49b57b85e+8df26ee1f0,gca7fc764a6+bcc48a0b46,gd7ef33dd92+bcc48a0b46,gdab6d2f7ff+422380537a,ge1c02a5578+b0138be388,ge410e46f29+bcc48a0b46,ge80df9fc40+e6db5413d1,geaed405ab2+1de65a85c6,gf5dcc679e7+35a0ce2edd,gf5f1c85443+e8e946ae08
LSST Data Management Base Package
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data.cc
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1/*
2 * This file is part of gauss2d_fit.
3 *
4 * Developed for the LSST Data Management System.
5 * This product includes software developed by the LSST Project
6 * (https://www.lsst.org).
7 * See the COPYRIGHT file at the top-level directory of this distribution
8 * for details of code ownership.
9 *
10 * This program is free software: you can redistribute it and/or modify
11 * it under the terms of the GNU General Public License as published by
12 * the Free Software Foundation, either version 3 of the License, or
13 * (at your option) any later version.
14 *
15 * This program is distributed in the hope that it will be useful,
16 * but WITHOUT ANY WARRANTY; without even the implied warranty of
17 * MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
18 * GNU General Public License for more details.
19 *
20 * You should have received a copy of the GNU General Public License
21 * along with this program. If not, see <https://www.gnu.org/licenses/>.
22 */
23
24#include <memory>
25#include <string>
26
27#include <pybind11/pybind11.h>
28#include <pybind11/stl.h>
29
33#include "lsst/gauss2d/python/image.h"
34
35#include "pybind11.h"
36
37namespace py = pybind11;
38using namespace pybind11::literals;
39
40namespace g2f = lsst::gauss2d::fit;
41namespace g2p = lsst::gauss2d::python;
42
43template <typename T>
44void declare_data(py::module &m, std::string str_type) {
47 std::string pyclass_name = std::string("Data") + str_type;
48 py::classh<Data, g2f::Chromatic, g2f::Parametric>(m, pyclass_name.c_str())
49 .def(py::init<std::vector<std::shared_ptr<const Observation>>>(), "data"_a)
50 .def_property_readonly("channels", &Data::get_channels)
51 .def("parameters", &Data::get_parameters, "parameters"_a = g2f::ParamRefs(),
52 "paramfilter"_a = nullptr)
53 .def_property_readonly("size", &Data::size)
54 .def("__getitem__", &Data::at)
55 .def("__len__", &Data::size)
56 // .def("__repr__", [](const Data &self) { return self.repr(true);
57 // })
58 .def("__str__", [str_type](const Data &self) {
59 std::string str = self.str();
61 self.CC_NAMESPACE_SEPARATOR);
62 return str;
63 });
64}
65
66void bind_data(py::module &m) {
68 declare_data<float>(m, "F");
69}
T c_str(T... args)
A list of Observation instances that can be modelled.
Definition data.h:32
An observed single-channel image with an associated variance and mask.
Definition observation.h:35
A Python image using numpy arrrays for storage.
Definition image.h:72
void declare_data(py::module &m, std::string str_type)
Definition data.cc:44
void bind_data(py::module &m)
Definition data.cc:66
std::vector< ParamBaseRef > ParamRefs
Definition param_defs.h:13
std::string replace_images_types(std::string target, std::string str_type, std::string_view separator)
Replace templated Image and index Image type name with Pythonic names.
Definition image.h:144