Coverage for python / lsst / multiprofit / priors.py: 55%
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« prev ^ index » next coverage.py v7.13.5, created at 2026-04-14 23:46 +0000
1# This file is part of multiprofit.
2#
3# Developed for the LSST Data Management System.
4# This product includes software developed by the LSST Project
5# (https://www.lsst.org).
6# See the COPYRIGHT file at the top-level directory of this distribution
7# for details of code ownership.
8#
9# This program is free software: you can redistribute it and/or modify
10# it under the terms of the GNU General Public License as published by
11# the Free Software Foundation, either version 3 of the License, or
12# (at your option) any later version.
13#
14# This program is distributed in the hope that it will be useful,
15# but WITHOUT ANY WARRANTY; without even the implied warranty of
16# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
17# GNU General Public License for more details.
18#
19# You should have received a copy of the GNU General Public License
20# along with this program. If not, see <https://www.gnu.org/licenses/>.
22__all__ = ["ShapePriorConfig", "get_hst_size_prior"]
24import lsst.gauss2d.fit as g2f
25import lsst.pex.config as pexConfig
26import numpy as np
28from .transforms import transforms_ref
31class ShapePriorConfig(pexConfig.Config):
32 """Configuration for a shape prior."""
34 prior_axrat_mean = pexConfig.Field[float](
35 default=0.7,
36 doc="Prior mean for axis ratio (prior ignored if not >0)",
37 )
38 prior_axrat_stddev = pexConfig.Field[float](
39 default=0,
40 doc="Prior std. dev. on axis ratio",
41 )
42 prior_size_mean = pexConfig.Field[float](
43 default=1,
44 doc="Prior mean for size_major",
45 )
46 prior_size_stddev = pexConfig.Field[float](
47 default=0,
48 doc="Prior std. dev. on size_major (prior ignored if not >0)",
49 )
51 def make_shape_prior(self, ellipse: g2f.ParametricEllipse) -> g2f.ShapePrior | None:
52 """Make a prior on ellipse (shape) parameters.
54 Parameters
55 ----------
56 ellipse
57 The ellipse to make a prior for.
59 Returns
60 -------
61 prior
62 The prior, or None if no positive stddev configured.
63 """
64 use_prior_axrat = (self.prior_axrat_stddev > 0) and np.isfinite(self.prior_axrat_stddev)
65 use_prior_size = (self.prior_size_stddev > 0) and np.isfinite(self.prior_size_stddev)
67 if use_prior_axrat or use_prior_size:
68 prior_size = (
69 g2f.ParametricGaussian1D(
70 g2f.MeanParameterD(self.prior_size_mean, transform=transforms_ref["log10"]),
71 g2f.StdDevParameterD(self.prior_size_stddev),
72 )
73 if use_prior_size
74 else None
75 )
76 prior_axrat = (
77 g2f.ParametricGaussian1D(
78 g2f.MeanParameterD(self.prior_axrat_mean, transform=transforms_ref["logit_axrat_prior"]),
79 g2f.StdDevParameterD(self.prior_axrat_stddev),
80 )
81 if use_prior_axrat
82 else None
83 )
84 return g2f.ShapePrior(ellipse, prior_size, prior_axrat)
85 return None
88def get_hst_size_prior(mag_psf_i: float) -> float:
89 """Return the mean and stddev for an HST-based size prior.
91 The size is major axis half-light radius.
93 Parameters
94 ----------
95 mag_psf_i
96 The i-band PSF magnitudes of the source(s).
98 Notes
99 -----
100 Return values are log10 scaled in units of arcseconds.
101 The input should be a PSF mag because other magnitudes - even Gaussian -
102 can be unreliable for low S/N (non-)detections.
103 """
104 return 0.75 * (19 - np.clip(mag_psf_i, 10, 30)) / 6.5, 0.2