Coverage for python/lsst/images/fields/_chebyshev.py: 22%

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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. 

11 

12from __future__ import annotations 

13 

14__all__ = ("ChebyshevField", "ChebyshevFieldSerializationModel") 

15 

16from collections.abc import Iterator 

17from typing import TYPE_CHECKING, Any, Literal, final 

18 

19import astropy.units 

20import numpy as np 

21import pydantic 

22 

23from .._concrete_bounds import SerializableBounds 

24from .._geom import YX, Bounds, Box 

25from .._image import Image 

26from ..serialization import ArchiveTree, InlineArray, InputArchive, InvalidParameterError, OutputArchive, Unit 

27from ._base import BaseField 

28 

29if TYPE_CHECKING: 

30 try: 

31 from lsst.afw.math import BackgroundMI as LegacyBackground 

32 from lsst.afw.math import ChebyshevBoundedField as LegacyChebyshevBoundedField 

33 except ImportError: 

34 type LegacyBackground = Any # type: ignore[no-redef] 

35 type LegacyChebyshevBoundedField = Any # type: ignore[no-redef] 

36 

37 

38@final 

39class ChebyshevField(BaseField): 

40 """A 2-d Chebyshev polynomial over a rectangular region. 

41 

42 Parameters 

43 ---------- 

44 bounds 

45 The region where this field can be evaluated. The ``bbox`` of this 

46 region is grown by half a pixel on all sides and then used to remap 

47 coordinates to ``[-1, 1]x[-1, 1]``, which is the natural domain of a 

48 2-d Chebyshev polynomial. 

49 coefficients 

50 Coefficients for the 2-d Chebyshev polynomial of the first kind, as a 

51 2-d matrix in which element ``[p, q]`` corresponds to the coefficient 

52 of ``T_p(y) T_q(x)``. Will be set to read-only in place. 

53 unit 

54 Units of the field. 

55 """ 

56 

57 def __init__( 

58 self, bounds: Bounds, coefficients: np.ndarray, *, unit: astropy.units.UnitBase | None = None 

59 ): 

60 self._bounds = bounds 

61 self._coefficients = coefficients 

62 self._coefficients.flags.writeable = False 

63 self._unit = unit 

64 # Compute the scaling and translation that map points in the bbox 

65 # (including an extra 0.5 on all sides, since the bbox is int-based) 

66 # to [-1, 1]. 

67 bbox = bounds.bbox 

68 self._xs = 2.0 / bbox.x.size 

69 self._xt = bbox.x.min + 0.5 * bbox.x.size - 0.5 

70 self._ys = 2.0 / bbox.y.size 

71 self._yt = bbox.y.min + 0.5 * bbox.y.size - 0.5 

72 

73 @staticmethod 

74 def fit( 

75 bounds: Bounds, 

76 data: np.ndarray | astropy.units.Quantity, 

77 order: int | None = None, 

78 *, 

79 y: np.ndarray, 

80 x: np.ndarray, 

81 weight: np.ndarray | None = None, 

82 y_order: int | None = None, 

83 x_order: int | None = None, 

84 triangular: bool = True, 

85 unit: astropy.units.UnitBase | None = None, 

86 ) -> ChebyshevField: 

87 """Fit a Chebyshev field to data points using linear least squares. 

88 

89 Parameters 

90 ---------- 

91 data 

92 Data points to fit. If this is an `astropy.units.Quantity`, 

93 this sets the units of the field and the ``unit`` argument cannot 

94 also be provided. 

95 order 

96 Maximum order for the Chebyshev polynomial in both dimensions. 

97 y 

98 Y coordinates of the data points. Must have either the same 

99 shape as ``data`` (providing the coordinates for all points 

100 directly), or be a 1-d array with the same size as 

101 ``data.shape[0]`` (when ``data`` is a 2-d image and ``y`` provides 

102 the coordinates of the rows). 

103 x 

104 X coordinates of the data points. Must have either the same 

105 shape as ``data`` (providing the coordinates for all points 

106 directly), or be a 1-d array with the same size as 

107 ``data.shape[1]`` (when ``data`` is a 2-d image and ``x`` provides 

108 the coordinates of the columns). 

109 weight 

110 Weights to apply to the data points. Must have the same shape as 

111 ``data``. 

112 y_order 

113 Maximum order for the Chebyshev polynomial in ``y``. Requires 

114 ``x_order`` to also be provided. Incompatible with ``order``. 

115 x_order 

116 Maximum order for the Chebyshev polynomial in ``x``. Requires 

117 ``y_order`` to also be provided. Incompatible with ``order``. 

118 triangular 

119 If `True`, only fit for coefficients of ``T_p(y) T_q(x)`` where 

120 ``p + q <= max(y_order, x_order)``. 

121 unit 

122 Units of the returned field. 

123 """ 

124 match (order, x_order, y_order): 

125 case (int(), None, None): 

126 x_order = order 

127 y_order = order 

128 case (None, int(), int()): 

129 pass 

130 case _: 

131 raise TypeError("Either 'order' (only) or both 'x_order' and 'y_order' must be provided.") 

132 if weight is not None and weight.shape != data.shape: 

133 raise ValueError(f"Shape of 'data' {data.shape} does not match 'weight' {weight.shape}.") 

134 if isinstance(data, astropy.units.Quantity): 

135 if unit is not None: 

136 raise TypeError("If 'data' is a Quantity, 'unit' cannot be provided separately.") 

137 unit = data.unit 

138 data = data.to_value() 

139 result = ChebyshevField(bounds, np.zeros((y_order + 1, x_order + 1), dtype=np.float64), unit=unit) 

140 if len(data.shape) == 2 and len(x.shape) == 1 and len(y.shape) == 1: 

141 if data.shape != y.shape + x.shape: 

142 raise ValueError( 

143 f"Shape of 2-d 'data' {data.shape} does not match 1-d 'y' {y.shape} and/or 'x' {x.shape}." 

144 ) 

145 matrix = result._make_grid_matrix(x=x, y=y, triangular=triangular) 

146 else: 

147 if data.shape != y.shape: 

148 raise ValueError(f"Shape of 'data' {data.shape} does not match 'y' {y.shape}.") 

149 if data.shape != x.shape: 

150 raise ValueError(f"Shape of 'data' {data.shape} does not match 'x' {x.shape}.") 

151 matrix = result._make_general_matrix(x=x, y=y, triangular=triangular) 

152 if weight is not None: 

153 weight = weight.ravel() # copies only if needed 

154 matrix *= weight[:, np.newaxis] 

155 data = data.flatten() # always copies 

156 data *= weight 

157 mask = np.logical_and(weight > 0, np.isfinite(data)) 

158 else: 

159 data = data.ravel() 

160 mask = np.isfinite(data) 

161 n_good = mask.sum() 

162 if n_good == 0: 

163 raise ValueError("No good data points.") 

164 if n_good < data.size: 

165 data = data[mask] 

166 matrix = matrix[mask, :] 

167 packed_coefficients, *_ = np.linalg.lstsq(matrix, data) 

168 result._coefficients.flags.writeable = True 

169 for i, pq in result._packing_indices(triangular): 

170 result._coefficients[pq.y, pq.x] = packed_coefficients[i] 

171 result._coefficients.flags.writeable = False 

172 return result 

173 

174 @property 

175 def bounds(self) -> Bounds: 

176 return self._bounds 

177 

178 @property 

179 def unit(self) -> astropy.units.UnitBase | None: 

180 return self._unit 

181 

182 @property 

183 def x_order(self) -> int: 

184 """Maximum polynomial order in the column dimension (`int`).""" 

185 return self._coefficients.shape[1] - 1 

186 

187 @property 

188 def y_order(self) -> int: 

189 """Maximum polynomial order in the row dimension (`int`).""" 

190 return self._coefficients.shape[0] - 1 

191 

192 @property 

193 def order(self) -> int: 

194 """Maximum polynomial order in either dimension (`int`).""" 

195 return max(self.x_order, self.y_order) 

196 

197 @property 

198 def coefficients(self) -> np.ndarray: 

199 """Coefficients for the 2-d Chebyshev polynomial of the first kind, 

200 as a 2-d matrix in which element ``[p, q]`` corresponds to the 

201 coefficient of ``T_p(y) T_q(x)``. 

202 """ 

203 return self._coefficients 

204 

205 @property 

206 def is_constant(self) -> bool: 

207 return self.x_order == 0 and self.y_order == 0 

208 

209 def evaluate( 

210 self, *, x: np.ndarray, y: np.ndarray, quantity: bool 

211 ) -> np.ndarray | astropy.units.Quantity: 

212 m = self._remap(x=x.copy(), y=y.copy()) 

213 # We swap x and y relative to Numpy's docs because that's how our 

214 # coefficients are ordered. 

215 v = np.polynomial.chebyshev.chebval2d(m.y, m.x, self._coefficients) 

216 if quantity: 

217 return astropy.units.Quantity(v, self.unit) 

218 return v 

219 

220 def render(self, bbox: Box | None = None, *, dtype: np.typing.DTypeLike | None = None) -> Image: 

221 if bbox is None: 

222 bbox = self.bounds.bbox 

223 m = self._remap( 

224 x=bbox.x.arange.astype(np.float64), 

225 y=bbox.y.arange.astype(np.float64), 

226 ) 

227 # We swap x and y relative to Numpy's docs because that's how our 

228 # coefficients and images are ordered. 

229 v = np.polynomial.chebyshev.chebgrid2d(m.y, m.x, self._coefficients) 

230 return Image(v, bbox=bbox, unit=self.unit, dtype=dtype) 

231 

232 def multiply_constant( 

233 self, factor: float | astropy.units.Quantity | astropy.units.UnitBase 

234 ) -> ChebyshevField: 

235 factor, unit = self._handle_factor_units(factor) 

236 return ChebyshevField(self.bounds, self.coefficients * factor, unit=unit) 

237 

238 def serialize(self, archive: OutputArchive[Any]) -> ChebyshevFieldSerializationModel: 

239 """Serialize the Chebyshev field to an output archive.""" 

240 return ChebyshevFieldSerializationModel( 

241 bounds=self.bounds.serialize(), 

242 coefficients=self.coefficients, 

243 unit=self.unit, 

244 ) 

245 

246 @staticmethod 

247 def _get_archive_tree_type( 

248 pointer_type: type[Any], 

249 ) -> type[ChebyshevFieldSerializationModel]: 

250 """Return the serialization model type for this object for an archive 

251 type that uses the given pointer type. 

252 """ 

253 return ChebyshevFieldSerializationModel 

254 

255 @staticmethod 

256 def from_legacy( 

257 legacy: LegacyChebyshevBoundedField, 

258 unit: astropy.units.UnitBase | None = None, 

259 bounds: Bounds | None = None, 

260 ) -> ChebyshevField: 

261 """Convert from a legacy `lsst.afw.math.ChebyshevBoundedField`. 

262 

263 Parameters 

264 ---------- 

265 legacy 

266 Legacy field to convert. 

267 unit 

268 The units of the returned field (`lsst.afw.math.BoundedField` 

269 objects do not know their units). 

270 bounds 

271 The bounds of the returned field, if they should be different from 

272 the bounding box of ``legacy``. 

273 """ 

274 bbox = Box.from_legacy(legacy.getBBox()) 

275 if bounds is not None: 

276 if bounds.bbox != bbox: 

277 raise ValueError( 

278 "Custom bounds when converting a ChebyshevBoundedField must not change the bbox." 

279 ) 

280 else: 

281 bounds = bbox 

282 return ChebyshevField(bounds=bounds, coefficients=legacy.getCoefficients(), unit=unit) 

283 

284 def to_legacy(self) -> LegacyChebyshevBoundedField: 

285 """Convert to a legacy `lsst.afw.math.ChebyshevBoundedField`.""" 

286 from lsst.afw.math import ChebyshevBoundedField as LegacyChebyshevBoundedField 

287 

288 return LegacyChebyshevBoundedField(self.bounds.bbox.to_legacy(), self.coefficients) 

289 

290 @staticmethod 

291 def from_legacy_background( 

292 legacy_background: LegacyBackground, 

293 bounds: Bounds | None = None, 

294 unit: astropy.units.UnitBase | None = None, 

295 ) -> ChebyshevField: 

296 """Convert from a legacy `lsst.afw.math.BackgroundMI` instance. 

297 

298 Parameters 

299 ---------- 

300 legacy 

301 Legacy background object to convert. 

302 bounds 

303 The bounds of the returned field, if they should be different from 

304 the bounding box of ``legacy_background``. 

305 unit 

306 The units of the returned field (`lsst.afw.math.Background` 

307 objects do not know their units). 

308 """ 

309 from lsst.afw.math import ApproximateControl 

310 

311 approx_control = legacy_background.getBackgroundControl().getApproximateControl() 

312 stats_image = legacy_background.getStatsImage() 

313 if approx_control.getStyle() != ApproximateControl.CHEBYSHEV: 

314 raise TypeError("Legacy background does not use Chebyshev approximation.") 

315 if approx_control.getWeighting(): 

316 weight = stats_image.variance.array ** (-0.5) 

317 else: 

318 weight = None 

319 x = legacy_background.getBinCentersX() 

320 y = legacy_background.getBinCentersY() 

321 bbox = Box.from_legacy(legacy_background.getImageBBox()) 

322 if bounds is not None: 

323 if bounds.bbox != bbox: 

324 raise ValueError( 

325 "Custom bounds when converting a Chebyshev background must not change the bbox." 

326 ) 

327 else: 

328 bounds = bbox 

329 return ChebyshevField.fit( 

330 bounds, 

331 stats_image.image.array, 

332 x=x, 

333 y=y, 

334 x_order=approx_control.getOrderX(), 

335 y_order=approx_control.getOrderY(), 

336 weight=weight, 

337 unit=unit, 

338 ) 

339 

340 def _remap(self, *, x: np.ndarray, y: np.ndarray) -> YX[np.ndarray]: 

341 x -= self._xt 

342 x *= self._xs 

343 y -= self._yt 

344 y *= self._ys 

345 return YX(y=y, x=x) 

346 

347 def _packing_indices(self, triangular: bool) -> Iterator[tuple[int, YX[int]]]: 

348 i = 0 

349 for p in range(self.y_order + 1): 

350 for q in range(self.x_order + 1): 

351 if not triangular or p + q <= self.order: 

352 yield i, YX(y=p, x=q) 

353 i += 1 

354 

355 def _make_grid_matrix(self, *, x: np.ndarray, y: np.ndarray, triangular: bool) -> np.ndarray: 

356 r = self._remap( 

357 x=np.asarray(x, dtype=np.float64, copy=True), 

358 y=np.asarray(y, dtype=np.float64, copy=True), 

359 ) 

360 yv = np.polynomial.chebyshev.chebvander(r.y, self.y_order) 

361 xv = np.polynomial.chebyshev.chebvander(r.x, self.x_order) 

362 indices = list(self._packing_indices(triangular)) 

363 tensor = np.zeros(r.y.shape + r.x.shape + (len(indices),), dtype=np.float64) 

364 for i, pq in indices: 

365 tensor[:, :, i] = np.multiply.outer(yv[:, pq.y], xv[:, pq.x]) 

366 return tensor.reshape(y.shape[0] * x.shape[0], len(indices)) 

367 

368 def _make_general_matrix(self, *, x: np.ndarray, y: np.ndarray, triangular: bool) -> np.ndarray: 

369 r = self._remap( 

370 x=np.asarray(x, dtype=np.float64, copy=True).ravel(), 

371 y=np.asarray(y, dtype=np.float64, copy=True).ravel(), 

372 ) 

373 yv = np.polynomial.chebyshev.chebvander(r.y, self.y_order) 

374 xv = np.polynomial.chebyshev.chebvander(r.x, self.x_order) 

375 indices = list(self._packing_indices(triangular)) 

376 matrix = np.zeros(r.y.shape + (len(indices),), dtype=np.float64) 

377 for i, pq in indices: 

378 matrix[:, i] = yv[:, pq.y] * xv[:, pq.x] 

379 return matrix 

380 

381 

382class ChebyshevFieldSerializationModel(ArchiveTree): 

383 """Serialization model for `ChebyshevField`.""" 

384 

385 bounds: SerializableBounds = pydantic.Field( 

386 description=( 

387 "The region where this field can be evaluated. " 

388 "The bbox of this region is grown by half a pixel on all sides and then used to remap " 

389 "coordinates to [-1, 1]x[-1, 1], which is the natural domain of a 2-d Chebyshev polynomial." 

390 ) 

391 ) 

392 

393 coefficients: InlineArray = pydantic.Field( 

394 description=( 

395 "Coefficients for a 2-d Chebyshev polynomial of the first kind, as a 2-d matrix in which " 

396 "element [p, q] corresponds to the coefficient of T_p(y) T_q(x)." 

397 ) 

398 ) 

399 

400 unit: Unit | None = pydantic.Field(default=None, description="Units of the field.") 

401 

402 field_type: Literal["CHEBYSHEV"] = "CHEBYSHEV" 

403 

404 def deserialize(self, archive: InputArchive, **kwargs: Any) -> ChebyshevField: 

405 """Deserialize the Chebyshev field from an input archive.""" 

406 if kwargs: 

407 raise InvalidParameterError(f"Unrecognized parameters for ChebyshevField: {set(kwargs.keys())}.") 

408 return ChebyshevField(self.bounds.deserialize(), self.coefficients, unit=self.unit)