Coverage for python/lsst/images/cells/_provenance.py: 44%
164 statements
« prev ^ index » next coverage.py v7.14.3, created at 2026-07-09 02:27 -0700
« prev ^ index » next coverage.py v7.14.3, created at 2026-07-09 02:27 -0700
1# This file is part of lsst-images.
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# Use of this source code is governed by a 3-clause BSD-style
10# license that can be found in the LICENSE file.
12from __future__ import annotations
14__all__ = ("CoaddProvenance", "CoaddProvenanceSerializationModel")
16from collections.abc import Iterable
17from typing import TYPE_CHECKING, Any, ClassVar
19import astropy.table
20import astropy.units as u
21import numpy as np
22import pydantic
24from .._cell_grid import CellIJ
25from .._polygon import Polygon
26from ..serialization import ArchiveTree, InputArchive, InvalidParameterError, OutputArchive, TableModel
28if TYPE_CHECKING:
29 try:
30 from lsst.afw.geom import Polygon as LegacyPolygon
31 from lsst.cell_coadds import CoaddInputs as LegacyCellCoaddInputs
32 from lsst.cell_coadds import MultipleCellCoadd as LegacyMultipleCellCoadd
33 from lsst.cell_coadds import ObservationIdentifiers as LegacyObservationIdentifiers
34 from lsst.skymap import Index2D as LegacyIndex2D
35 except ImportError:
36 type LegacyIndex2D = Any # type: ignore[no-redef]
37 type LegacyCellCoaddInputs = Any # type: ignore[no-redef]
38 type LegacyPolygon = Any # type: ignore[no-redef]
39 type LegacyMultipleCellCoadd = Any # type: ignore[no-redef]
40 type LegacyObservationIdentifiers = Any # type: ignore[no-redef]
43class CoaddProvenance:
44 """A pair of tables that record the inputs to a cell-based coadd.
46 Parameters
47 ----------
48 inputs
49 A table of {visit, detector} combinations that contribute to any cell
50 in the coadd.
51 contributions
52 A table of {visit, detector, cell} combinations that describe how an
53 observation contributed to a cell.
55 Notes
56 -----
57 This object can represent the provenance of a whole patch, a single cell,
58 or anything in between. In the single-cell case, the ``inputs`` and
59 ``contributions`` tables have the same number of rows (but may not be
60 ordered the same way!).
61 """
63 def __init__(self, inputs: astropy.table.Table, contributions: astropy.table.Table) -> None:
64 self._inputs = inputs
65 self._contributions = contributions
67 _INPUT_TABLE_COLUMNS: ClassVar[list[tuple[str, type, str]]] = [
68 ("instrument", np.object_, "Name of the instrument."),
69 ("visit", np.uint64, "ID of the visit."),
70 ("detector", np.uint16, "ID of the detector."),
71 ("physical_filter", np.object_, "Full name of the bandpass filter."),
72 ("day_obs", np.uint32, "Observation night as a YYYYMMDD integer."),
73 (
74 "polygon",
75 np.object_,
76 (
77 "Polygon that approximates the overlap of the observation and the coadd patch, "
78 "in coadd coordinates."
79 ),
80 ),
81 ]
83 _CONTRIBUTION_TABLE_COLUMNS: ClassVar[list[tuple[str, type, str, u.UnitBase | None]]] = [
84 ("cell_i", np.uint16, "Y-axis index of the cell within the patch.", None),
85 ("cell_j", np.uint16, "X-axis index of the cell within the patch.", None),
86 ("instrument", np.object_, "Name of the instrument.", None),
87 ("visit", np.uint64, "ID of the visit.", None),
88 ("detector", np.uint16, "ID of the detector.", None),
89 ("overlaps_center", np.bool_, "Whether a this observation overlaps the center of the cell.", None),
90 ("overlap_fraction", np.float64, "Fraction of the cell that is covered by the overlap region.", None),
91 ("unmasked_fraction", np.float64, "Fraction of the cell propagated to the coadd.", None),
92 ("weight", np.float64, "Weight to be used for this input in this cell.", None),
93 ("psf_shape_xx", np.float64, "Second order moments of the PSF.", u.pix**2),
94 ("psf_shape_yy", np.float64, "Second order moments of the PSF.", u.pix**2),
95 ("psf_shape_xy", np.float64, "Second order moments of the PSF.", u.pix**2),
96 (
97 "psf_shape_flag",
98 np.bool_,
99 "Flag indicating whether the PSF shape measurement was successful.",
100 None,
101 ),
102 ]
104 @classmethod
105 def make_empty_input_table(cls, n_rows: int) -> astropy.table.Table:
106 """Make an empty `inputs` table with a set number of rows.
108 Parameters
109 ----------
110 n_rows
111 Number of rows in the new table.
112 """
113 return astropy.table.Table(
114 [
115 astropy.table.Column(name=name, length=n_rows, dtype=dtype, description=description)
116 for name, dtype, description in cls._INPUT_TABLE_COLUMNS
117 ]
118 )
120 @classmethod
121 def make_empty_contribution_table(cls, n_rows: int) -> astropy.table.Table:
122 """Make an empty `contributions` table with a set number of rows.
124 Parameters
125 ----------
126 n_rows
127 Number of rows in the new table.
128 """
129 return astropy.table.Table(
130 [
131 astropy.table.Column(
132 name=name, length=n_rows, dtype=dtype, description=description, unit=unit
133 )
134 for name, dtype, description, unit in cls._CONTRIBUTION_TABLE_COLUMNS
135 ]
136 )
138 @property
139 def inputs(self) -> astropy.table.Table:
140 """A table of {visit, detector} combinations that contribute to any
141 cell in the coadd.
142 """
143 return self._inputs
145 @property
146 def contributions(self) -> astropy.table.Table:
147 """A table of {visit, detector, cell} combinations that describe how an
148 observation contributed to a cell.
149 """
150 return self._contributions
152 def __getitem__(self, cell: CellIJ) -> CoaddProvenance:
153 return self.subset([cell])
155 def subset(self, cells: Iterable[CellIJ]) -> CoaddProvenance:
156 """Return a new provenance object with just the given cells.
158 Parameters
159 ----------
160 cells
161 Cells to keep in the returned provenance.
162 """
163 cells_to_keep = astropy.table.Table(
164 rows=[(index.i, index.j) for index in cells],
165 names=["cell_i", "cell_j"],
166 dtype=[np.uint16, np.uint16],
167 )
168 contributions = astropy.table.join(self._contributions, cells_to_keep)
169 assert contributions.columns.keys() == {name for name, _, _, _ in self._CONTRIBUTION_TABLE_COLUMNS}
170 inputs = astropy.table.join(contributions["instrument", "visit", "detector"], self._inputs)
171 assert inputs.columns.keys() == {name for name, _, _ in self._INPUT_TABLE_COLUMNS}
172 return CoaddProvenance(inputs=inputs, contributions=contributions)
174 def serialize(self, archive: OutputArchive[Any]) -> CoaddProvenanceSerializationModel:
175 """Serialize the provenance to an output archive.
177 Parameters
178 ----------
179 archive
180 Archive to write to.
181 """
182 inputs = self._inputs.copy(copy_data=False)
183 contributions = self._contributions.copy(copy_data=False)
184 instrument = CoaddProvenanceSerializationModel._fix_str_for_serialization(
185 "instrument", inputs, contributions
186 )
187 physical_filter = CoaddProvenanceSerializationModel._fix_str_for_serialization(
188 "physical_filter", inputs
189 )
190 CoaddProvenanceSerializationModel._fix_polygon_for_serialization(inputs)
191 inputs_model = archive.add_table(inputs, name="inputs")
192 contributions_model = archive.add_table(contributions, name="contributions")
193 return CoaddProvenanceSerializationModel(
194 instrument=instrument,
195 physical_filter=physical_filter,
196 inputs=inputs_model,
197 contributions=contributions_model,
198 )
200 @staticmethod
201 def from_legacy(legacy_cell_coadd: LegacyMultipleCellCoadd) -> CoaddProvenance:
202 """Extract provenance from a legacy
203 `lsst.cell_coadds.MultipleCellCoadd` object.
205 Parameters
206 ----------
207 legacy_cell_coadd
208 Legacy cell coadd to extract provenance from.
209 """
210 inputs = CoaddProvenance.make_empty_input_table(len(legacy_cell_coadd.common.visit_polygons))
211 for n, (legacy_identifiers, legacy_polygon) in enumerate(
212 legacy_cell_coadd.common.visit_polygons.items()
213 ):
214 inputs["instrument"][n] = legacy_identifiers.instrument
215 inputs["visit"][n] = legacy_identifiers.visit
216 inputs["detector"][n] = legacy_identifiers.detector
217 inputs["physical_filter"][n] = legacy_identifiers.physical_filter
218 inputs["day_obs"][n] = legacy_identifiers.day_obs
219 inputs["polygon"][n] = Polygon.from_legacy(legacy_polygon)
220 n_contributions = 0
221 for legacy_cell in legacy_cell_coadd.cells.values():
222 n_contributions += len(legacy_cell.inputs)
223 contributions = CoaddProvenance.make_empty_contribution_table(n_contributions)
224 n = 0
225 for legacy_cell in legacy_cell_coadd.cells.values():
226 for legacy_identifiers, legacy_inputs in legacy_cell.inputs.items():
227 contributions["cell_i"][n] = legacy_cell.identifiers.cell.y
228 contributions["cell_j"][n] = legacy_cell.identifiers.cell.x
229 contributions["instrument"][n] = legacy_identifiers.instrument
230 contributions["visit"][n] = legacy_identifiers.visit
231 contributions["detector"][n] = legacy_identifiers.detector
232 contributions["overlaps_center"][n] = legacy_inputs.overlaps_center
233 contributions["overlap_fraction"][n] = legacy_inputs.overlap_fraction
234 contributions["unmasked_fraction"][n] = legacy_inputs.unmasked_overlap_fraction
235 contributions["weight"][n] = legacy_inputs.weight
236 contributions["psf_shape_xx"][n] = legacy_inputs.psf_shape.getIxx()
237 contributions["psf_shape_yy"][n] = legacy_inputs.psf_shape.getIyy()
238 contributions["psf_shape_xy"][n] = legacy_inputs.psf_shape.getIxy()
239 contributions["psf_shape_flag"][n] = legacy_inputs.psf_shape_flag
240 n += 1
241 return CoaddProvenance(inputs=inputs, contributions=contributions)
243 def to_legacy_polygon_map(self) -> dict[LegacyObservationIdentifiers, LegacyPolygon]:
244 """Construct a legacy mapping from
245 `lsst.cell_coadds.ObservationIdentifiers` to `lsst.afw.geom.Polygon`
246 from the `inputs` table.
247 """
248 from lsst.cell_coadds import ObservationIdentifiers as LegacyObservationIdentifiers
250 return {
251 LegacyObservationIdentifiers(
252 instrument=str(row["instrument"]),
253 physical_filter=str(row["physical_filter"]),
254 visit=int(row["visit"]),
255 day_obs=int(row["day_obs"]),
256 detector=int(row["detector"]),
257 ): row["polygon"].to_legacy()
258 for row in self.inputs
259 }
261 def to_legacy_cell_coadd_inputs(
262 self, observations: Iterable[LegacyObservationIdentifiers] | None
263 ) -> dict[LegacyIndex2D, dict[LegacyObservationIdentifiers, LegacyCellCoaddInputs]]:
264 """Construct a mapping from legacy cell index to the list of legacy
265 input structs for that cell.
267 Parameters
268 ----------
269 observations
270 Observations to include, or `None` to include all observations
271 in the `inputs` table.
272 """
273 from lsst.afw.geom.ellipses import Quadrupole
274 from lsst.cell_coadds import CoaddInputs as LegacyCoaddInputs
275 from lsst.skymap import Index2D as LegacyIndex2D
277 if observations is None:
278 observations = self.to_legacy_polygon_map().keys()
279 observations_by_key: dict[tuple[str, int, int], LegacyObservationIdentifiers] = {
280 (obs.instrument, obs.visit, obs.detector): obs for obs in observations
281 }
282 result: dict[LegacyIndex2D, dict[LegacyObservationIdentifiers, LegacyCoaddInputs]] = {}
283 for row in self.contributions:
284 obs_key = (str(row["instrument"]), int(row["visit"]), int(row["detector"]))
285 obs = observations_by_key[obs_key]
286 cell_inputs = result.setdefault(LegacyIndex2D(x=int(row["cell_j"]), y=int(row["cell_i"])), {})
287 cell_inputs[obs] = LegacyCoaddInputs(
288 overlaps_center=bool(row["overlaps_center"]),
289 overlap_fraction=float(row["overlap_fraction"]),
290 unmasked_overlap_fraction=float(row["unmasked_fraction"]),
291 weight=float(row["weight"]),
292 psf_shape=Quadrupole(row["psf_shape_xx"], row["psf_shape_yy"], row["psf_shape_xy"]),
293 psf_shape_flag=bool(row["psf_shape_flag"]),
294 )
295 return result
298class CoaddProvenanceSerializationModel(ArchiveTree):
299 """A Pydantic model used to represent a serialized `CoaddProvenance`.
301 Notes
302 -----
303 We can't rewrite the Astropy tables directly into the archive (e.g. as
304 FITS binary tables for a FITS archive), because:
306 - `str` columns are a huge pain in both Numpy and FITS;
307 - the polygon columns need to be rewritten as array-valued columns.
309 To deal with the string columns (``instrument`` and ``physical_filter``)
310 we do dictionary compression: we map each distinct value of those columns
311 to an integer, and then we save that mapping to the model while saving
312 an integer version of that column in the table. But if there is actually
313 only one value in that column (the most common case by far) we just drop
314 the column and store that value directly in the model.
315 """
317 SCHEMA_NAME: ClassVar[str] = "coadd_provenance"
318 SCHEMA_VERSION: ClassVar[str] = "1.0.0"
319 MIN_READ_VERSION: ClassVar[int] = 1
320 PUBLIC_TYPE: ClassVar[type] = CoaddProvenance
322 instrument: str | dict[str, int] = pydantic.Field(
323 description=(
324 "Instrument name for all inputs to this coadd, or a mapping from "
325 "instrument name to the integer used in its place in the tables."
326 )
327 )
328 physical_filter: str | dict[str, int] = pydantic.Field(
329 description="Physical filter name for all inputs to this coadd."
330 )
331 inputs: TableModel = pydantic.Field(description="Table of all inputs to the coadd.")
332 contributions: TableModel = pydantic.Field(description="Table of per-cell contributions to the coadd.")
334 def deserialize(self, archive: InputArchive[Any], **kwargs: Any) -> CoaddProvenance:
335 """Deserialize a provenance from an input archive.
337 Parameters
338 ----------
339 archive
340 Archive to read from.
341 **kwargs
342 Unsupported keyword arguments are accepted only to provide
343 better error messages (raising
344 `.serialization.InvalidParameterError`).
346 Notes
347 -----
348 While `CoaddProvenance.subset` can be used to filter provenance
349 information down to just certain cells, there is no advantage to be
350 had from doing this during deserialization (the table data is not
351 ordered by cell, and hence there's read-slicing we can do).
352 """
353 if kwargs: 353 ↛ 354line 353 didn't jump to line 354 because the condition on line 353 was never true
354 raise InvalidParameterError(f"Unrecognized parameters for CoaddProvenance: {set(kwargs.keys())}.")
355 inputs = archive.get_table(self.inputs)
356 contributions = archive.get_table(self.contributions)
357 CoaddProvenanceSerializationModel._fix_str_for_deserialization(
358 "instrument", self.instrument, inputs, contributions
359 )
360 CoaddProvenanceSerializationModel._fix_str_for_deserialization(
361 "physical_filter", self.physical_filter, inputs
362 )
363 CoaddProvenanceSerializationModel._fix_polygon_for_deserialization(inputs)
364 for name, _, description in CoaddProvenance._INPUT_TABLE_COLUMNS:
365 inputs.columns[name].description = description
366 for name, _, description, unit in CoaddProvenance._CONTRIBUTION_TABLE_COLUMNS:
367 contributions.columns[name].description = description
368 contributions.columns[name].unit = unit
369 return CoaddProvenance(inputs=inputs, contributions=contributions)
371 @staticmethod
372 def _fix_str_for_serialization(column: str, *tables: astropy.table.Table) -> str | dict[str, int]:
373 """Rewrite a string column as an integer column or drop it.
375 Parameters
376 ----------
377 column
378 Name of the column to rewrite.
379 *tables
380 One or more astropy tables to rewrite. The first table is assumed
381 to have all values for this column that might appear in any other
382 tables.
384 Returns
385 -------
386 `str` | `dict` [`str`, `int`]
387 If there is only one unique value for this column in the first
388 table, that value (and the column will have been dropped from
389 all givne tables). If the tables are empty, the column is
390 dropped and an empty `dict` is returned. In all other cases the
391 given column is replaced with an integer column in all given
392 tables and the mapping from strings to integers is returned.
393 """
394 result: str | dict[str, int] = {name: n for n, name in enumerate(sorted(set(tables[0][column])))}
395 match len(result):
396 case 0:
397 pass
398 case 1:
399 (result,) = result.keys() # type: ignore[union-attr]
400 case _:
401 for table in tables:
402 table.columns[column] = astropy.table.Column(
403 data=[result[k] for k in table.columns[column]],
404 name=column,
405 dtype=np.uint8,
406 description=f"Integer mapped to {column} name.",
407 )
408 return result
409 # If we didn't remap to an integer (case 0 and 1 above), delete the
410 # column.
411 for table in tables:
412 del table.columns[column]
413 return result
415 @staticmethod
416 def _fix_str_for_deserialization(
417 column: str, value: str | dict[str, int], *tables: astropy.table.Table
418 ) -> None:
419 """Rewrite an integer column back to a string one.
421 Parameters
422 ----------
423 column
424 Name of the column to rewrite.
425 value
426 Value or mapping of values returned by
427 `_fix_str_for_serialization`.
428 tables
429 Tables to rewrite this column in.
430 """
431 match value:
432 case str(): 432 ↛ 435line 432 didn't jump to line 435 because the pattern on line 432 always matched
433 for table in tables:
434 table.columns[column] = astropy.table.Column([value] * len(table), dtype=object)
435 case dict():
436 mapping = {v: k for k, v in value.items()}
437 for table in tables:
438 table.columns[column] = astropy.table.Column(
439 [mapping[k] for k in table[column]], dtype=object
440 )
442 @staticmethod
443 def _fix_polygon_for_serialization(inputs: astropy.table.Table) -> None:
444 """Rewrite a polygon `object` column as a pair of array-valued columns
445 and an array-size column.
447 Parameters
448 ----------
449 inputs
450 A copy of the in-memory coadd inputs table to modify in-place into
451 its serialization form.
452 """
453 max_n_vertices = max(p.n_vertices for p in inputs["polygon"])
454 inputs["n_vertices"] = astropy.table.Column(
455 [p.n_vertices for p in inputs["polygon"]],
456 name="n_vertices",
457 dtype=np.uint8,
458 description="Number of polygon vertices.",
459 )
460 inputs["x_vertices"] = astropy.table.Column(
461 name="x_vertices",
462 dtype=np.float64,
463 length=len(inputs),
464 shape=(max_n_vertices,),
465 description="X coordinates of polygon vertices, in tract coordinates.",
466 )
467 inputs["x_vertices"][:, :] = np.nan
468 inputs["y_vertices"] = astropy.table.Column(
469 name="y_vertices",
470 dtype=np.float64,
471 length=len(inputs),
472 shape=(max_n_vertices,),
473 description="Y coordinates of polygon vertices, in tract coordinates.",
474 )
475 inputs["y_vertices"][:, :] = np.nan
476 for i, polygon in enumerate(inputs["polygon"]):
477 inputs["n_vertices"][i] = polygon.n_vertices
478 inputs["x_vertices"][i][: polygon.n_vertices] = polygon.x_vertices
479 inputs["y_vertices"][i][: polygon.n_vertices] = polygon.y_vertices
480 del inputs["polygon"]
482 @staticmethod
483 def _fix_polygon_for_deserialization(inputs: astropy.table.Table) -> None:
484 """Rewrite a a pair of array-valued columns and an array-size column
485 into a polygon `object` column.
487 Parameters
488 ----------
489 inputs
490 The serialized version of the coadd inputs table, to be modified
491 in-place into its in-memory form.
492 """
493 polygons = [
494 Polygon(x_vertices=x_vertices[:n_vertices], y_vertices=y_vertices[:n_vertices])
495 for n_vertices, x_vertices, y_vertices in zip(
496 inputs["n_vertices"], inputs["x_vertices"], inputs["y_vertices"]
497 )
498 ]
499 del inputs["n_vertices"]
500 del inputs["x_vertices"]
501 del inputs["y_vertices"]
502 inputs["polygon"] = astropy.table.Column(polygons, name="polygon", dtype=np.object_)