Coverage for python / lsst / analysis / tools / tasks / coaddDepthSummary.py: 32%
53 statements
« prev ^ index » next coverage.py v7.13.5, created at 2026-04-30 09:26 +0000
« prev ^ index » next coverage.py v7.13.5, created at 2026-04-30 09:26 +0000
1# This file is part of analysis_tools.
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/>.
21from __future__ import annotations
23__all__ = (
24 "CoaddDepthSummaryConfig",
25 "CoaddDepthSummaryTask",
26)
29import numpy as np
30from astropy.table import Table
32from lsst.pex.config import ListField
33from lsst.pipe.base import PipelineTask, PipelineTaskConfig, PipelineTaskConnections, Struct
34from lsst.pipe.base import connectionTypes as cT
37class CoaddDepthSummaryConnections(
38 PipelineTaskConnections,
39 dimensions=("tract", "skymap"),
40 defaultTemplates={"coaddName": ""}, # set as either deep or template in the pipeline
41):
42 data = cT.Input(
43 doc="Coadd n_image to load from the butler (pixel values are the number of input images).",
44 name="{coaddName}_coadd_n_image",
45 storageClass="ImageU",
46 multiple=True,
47 dimensions=("tract", "patch", "band", "skymap"),
48 deferLoad=True,
49 )
51 statTable = cT.Output(
52 doc="Table with resulting n_image based depth statistics.",
53 name="{coaddName}_coadd_depth_table",
54 storageClass="ArrowAstropy",
55 dimensions=("tract", "skymap"),
56 )
59class CoaddDepthSummaryConfig(PipelineTaskConfig, pipelineConnections=CoaddDepthSummaryConnections):
60 threshold_list = ListField(
61 default=[1, 2, 3, 5, 12],
62 dtype=int,
63 doc="The n_image pixel value thresholds, in ascending order.",
64 )
66 quantile_list = ListField(
67 default=[5, 10, 25, 50, 75, 90, 95],
68 dtype=int,
69 doc="The percentiles at which to compute n_image values, in ascending order.",
70 )
73class CoaddDepthSummaryTask(PipelineTask):
74 ConfigClass = CoaddDepthSummaryConfig
75 _DefaultName = "coaddDepthSummary"
77 def runQuantum(self, butlerQC, inputRefs, outputRefs):
78 inputs = butlerQC.get(inputRefs)
79 outputs = self.run(inputs)
80 butlerQC.put(outputs, outputRefs)
82 def run(self, inputs):
83 t = Table()
84 bands = []
85 patches = []
86 medians = []
87 stdevs = []
88 stats = []
89 quantiles = []
91 for n_image_handle in inputs["data"]:
92 n_image = n_image_handle.get()
93 data_id = n_image_handle.dataId
94 band = str(data_id.band.name)
95 patch = int(data_id.patch.id)
96 median = np.nanmedian(n_image.array)
97 stdev = np.nanstd(n_image.array)
99 bands.append(band)
100 patches.append(patch)
101 medians.append(median)
102 stdevs.append(stdev)
104 band_patch_stats = []
105 for threshold in self.config.threshold_list:
106 # Calculate the percentage of the image with an image depth
107 # above the given threshold.
108 stat = np.sum(n_image.array >= threshold) * 100 / (n_image.getHeight() * n_image.getWidth())
109 band_patch_stats.append(stat)
111 stats.append(band_patch_stats)
113 # Calculate the quantiles for image depth
114 # across the whole n_image array.
115 quantile = list(np.percentile(n_image.array, q=self.config.quantile_list))
116 quantiles.append(quantile)
118 threshold_col_names = [
119 f"depth_above_threshold_{threshold}" for threshold in self.config.threshold_list
120 ]
121 quantile_col_names = [f"depth_{q}_percentile" for q in self.config.quantile_list]
123 # Construct the Astropy table
124 data = [patches, bands, medians, stdevs] + list(zip(*stats)) + list(zip(*quantiles))
125 names = ["patch", "band", "medians", "stdevs"] + threshold_col_names + quantile_col_names
126 dtype = (
127 ["int", "str", "float", "float"]
128 + ["float" for x in range(len(list(zip(*stats))))]
129 + ["int" for y in range(len(list(zip(*quantiles))))]
130 )
131 t = Table(data=data, names=names, dtype=dtype)
132 return Struct(statTable=t)