Coverage for python / lsst / meas / base / forcedMeasurement.py: 25%

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21 

22r"""Base classes for forced measurement plugins and the driver task for these. 

23 

24In forced measurement, a reference catalog is used to define restricted 

25measurements (usually just fluxes) on an image. As the reference catalog may 

26be deeper than the detection limit of the measurement image, we do not assume 

27that we can use detection and deblend information from the measurement image. 

28Instead, we assume this information is present in the reference catalog and 

29can be "transformed" in some sense to the measurement frame. At the very 

30least, this means that `~lsst.afw.detection.Footprint`\ s from the reference 

31catalog should be transformed and installed as Footprints in the output 

32measurement catalog. If we have a procedure that can transform "heavy" 

33Footprints (ie, including pixel data), we can then proceed with measurement as 

34usual, but using the reference catalog's ``id`` and ``parent`` fields to 

35define deblend families. If this transformation does not preserve 

36heavy Footprints (this is currently the case, at least for CCD forced 

37photometry), then we will only be able to replace objects with noise one 

38deblend family at a time, and hence measurements run in single-object mode may 

39be contaminated by neighbors when run on objects with ``parent != 0``. 

40 

41Measurements are generally recorded in the coordinate system of the image 

42being measured (and all slot-eligible fields must be), but non-slot fields may 

43be recorded in other coordinate systems if necessary to avoid information loss 

44(this should, of course, be indicated in the field documentation). Note that 

45the reference catalog may be in a different coordinate system; it is the 

46responsibility of plugins to transform the data they need themselves, using 

47the reference WCS provided. However, for plugins that only require a position 

48or shape, they may simply use output `~lsst.afw.table.SourceCatalog`\'s 

49centroid or shape slots, which will generally be set to the transformed 

50position of the reference object before any other plugins are run, and hence 

51avoid using the reference catalog at all. 

52 

53Command-line driver tasks for forced measurement include 

54`ForcedPhotCcdTask`, and `ForcedPhotCoaddTask`. 

55""" 

56 

57import lsst.pex.config 

58import lsst.pipe.base 

59from lsst.utils.logging import PeriodicLogger 

60 

61from .pluginRegistry import PluginRegistry 

62from .baseMeasurement import (BaseMeasurementPluginConfig, BaseMeasurementPlugin, 

63 BaseMeasurementConfig, BaseMeasurementTask) 

64 

65__all__ = ("ForcedPluginConfig", "ForcedPlugin", 

66 "ForcedMeasurementConfig", "ForcedMeasurementTask") 

67 

68 

69class ForcedPluginConfig(BaseMeasurementPluginConfig): 

70 """Base class for configs of forced measurement plugins.""" 

71 

72 pass 

73 

74 

75class ForcedPlugin(BaseMeasurementPlugin): 

76 """Base class for forced measurement plugins. 

77 

78 Parameters 

79 ---------- 

80 config : `ForcedPlugin.ConfigClass` 

81 Configuration for this plugin. 

82 name : `str` 

83 The string with which the plugin was registered. 

84 schemaMapper : `lsst.afw.table.SchemaMapper` 

85 A mapping from reference catalog fields to output catalog fields. 

86 Output fields should be added to the output schema. While most plugins 

87 will not need to map fields from the reference schema, if they do so, 

88 those fields will be transferred before any plugins are run. 

89 metadata : `lsst.daf.base.PropertySet` 

90 Plugin metadata that will be attached to the output catalog. 

91 logName : `str`, optional 

92 Name to use when logging errors. 

93 """ 

94 

95 registry = PluginRegistry(ForcedPluginConfig) 

96 """Subclasses of `ForcedPlugin` must be registered here (`PluginRegistry`). 

97 """ 

98 

99 ConfigClass = ForcedPluginConfig 

100 

101 def __init__(self, config, name, schemaMapper, metadata, logName=None): 

102 BaseMeasurementPlugin.__init__(self, config, name, logName=logName) 

103 

104 def measure(self, measRecord, exposure, refRecord, refWcs): 

105 """Measure the properties of a source given an image and a reference. 

106 

107 Parameters 

108 ---------- 

109 exposure : `lsst.afw.image.ExposureF` 

110 The pixel data to be measured, together with the associated PSF, 

111 WCS, etc. All other sources in the image should have been replaced 

112 by noise according to deblender outputs. 

113 measRecord : `lsst.afw.table.SourceRecord` 

114 Record describing the object being measured. Previously-measured 

115 quantities will be retrieved from here, and it will be updated 

116 in-place with the outputs of this plugin. 

117 refRecord : `lsst.afw.table.SimpleRecord` 

118 Additional parameters to define the fit, as measured elsewhere. 

119 refWcs : `lsst.afw.geom.SkyWcs` or `lsst.afw.geom.Angle` 

120 The coordinate system for the reference catalog values. An 

121 `~lsst.geom.Angle` may be passed, indicating that a local tangent 

122 WCS should be created for each object using the given angle as a 

123 pixel scale. 

124 

125 Notes 

126 ----- 

127 In the normal mode of operation, the source centroid will be set to 

128 the WCS-transformed position of the reference object, so plugins that 

129 only require a reference position should not have to access the 

130 reference object at all. 

131 """ 

132 raise NotImplementedError() 

133 

134 def measureN(self, measCat, exposure, refCat, refWcs): 

135 """Measure the properties of blended sources from image & reference. 

136 

137 This operates on all members of a blend family at once. 

138 

139 Parameters 

140 ---------- 

141 exposure : `lsst.afw.image.ExposureF` 

142 The pixel data to be measured, together with the associated PSF, 

143 WCS, etc. Sources not in the blended hierarchy to be measured 

144 should have been replaced with noise using deblender outputs. 

145 measCat : `lsst.afw.table.SourceCatalog` 

146 Catalog describing the objects (and only those objects) being 

147 measured. Previously-measured quantities will be retrieved from 

148 here, and it will be updated in-place with the outputs of this 

149 plugin. 

150 refCat : `lsst.afw.table.SimpleCatalog` 

151 Additional parameters to define the fit, as measured elsewhere. 

152 Ordered such that ``zip(measCat, refcat)`` may be used. 

153 refWcs : `lsst.afw.geom.SkyWcs` or `lsst.afw.geom.Angle` 

154 The coordinate system for the reference catalog values. An 

155 `~lsst.geom.Angle` may be passed, indicating that a local tangent 

156 WCS should be created for each object using the given angle as a 

157 pixel scale. 

158 

159 Notes 

160 ----- 

161 In the normal mode of operation, the source centroids will be set to 

162 the WCS-transformed position of the reference object, so plugins that 

163 only require a reference position should not have to access the 

164 reference object at all. 

165 """ 

166 raise NotImplementedError() 

167 

168 

169class ForcedMeasurementConfig(BaseMeasurementConfig): 

170 """Config class for forced measurement driver task. 

171 """ 

172 

173 plugins = ForcedPlugin.registry.makeField( 

174 multi=True, 

175 default=["base_PixelFlags", 

176 "base_TransformedCentroid", 

177 "base_SdssCentroid", 

178 "base_TransformedShape", 

179 "base_SdssShape", 

180 "base_GaussianFlux", 

181 "base_CircularApertureFlux", 

182 "base_PsfFlux", 

183 "base_LocalBackground", 

184 ], 

185 doc="Plugins to be run and their configuration" 

186 ) 

187 algorithms = property(lambda self: self.plugins, doc="backwards-compatibility alias for plugins") 

188 undeblended = ForcedPlugin.registry.makeField( 

189 multi=True, 

190 default=[], 

191 doc="Plugins to run on undeblended image" 

192 ) 

193 copyColumns = lsst.pex.config.DictField( 

194 keytype=str, itemtype=str, doc="Mapping of reference columns to source columns", 

195 default={"id": "objectId", "parent": "parentObjectId", "deblend_nChild": "deblend_nChild", 

196 "coord_ra": "coord_ra", "coord_dec": "coord_dec"} 

197 ) 

198 checkUnitsParseStrict = lsst.pex.config.Field( 

199 doc="Strictness of Astropy unit compatibility check, can be 'raise', 'warn' or 'silent'", 

200 dtype=str, 

201 default="raise", 

202 ) 

203 

204 def setDefaults(self): 

205 self.slots.centroid = "base_TransformedCentroid" 

206 self.slots.shape = "base_TransformedShape" 

207 self.slots.apFlux = None 

208 self.slots.modelFlux = None 

209 self.slots.psfFlux = None 

210 self.slots.gaussianFlux = None 

211 self.slots.calibFlux = None 

212 

213 

214class ForcedMeasurementTask(BaseMeasurementTask): 

215 """Measure sources on an image, constrained by a reference catalog. 

216 

217 A subtask for measuring the properties of sources on a single image, 

218 using an existing "reference" catalog to constrain some aspects of the 

219 measurement. 

220 

221 Parameters 

222 ---------- 

223 refSchema : `lsst.afw.table.Schema` 

224 Schema of the reference catalog. Must match the catalog later passed 

225 to 'ForcedMeasurementTask.generateMeasCat` and/or 

226 `ForcedMeasurementTask.run`. 

227 algMetadata : `lsst.daf.base.PropertyList` or `None` 

228 Will be updated in place to to record information about each 

229 algorithm. An empty `~lsst.daf.base.PropertyList` will be created if 

230 `None`. 

231 **kwds 

232 Keyword arguments are passed to the supertask constructor. 

233 

234 Notes 

235 ----- 

236 Note that while `SingleFrameMeasurementTask` is passed an initial 

237 `~lsst.afw.table.Schema` that is appended to in order to create the output 

238 `~lsst.afw.table.Schema`, `ForcedMeasurementTask` is initialized with the 

239 `~lsst.afw.table.Schema` of the reference catalog, from which a new 

240 `~lsst.afw.table.Schema` for the output catalog is created. Fields to be 

241 copied directly from the reference `~lsst.afw.table.Schema` are added 

242 before ``Plugin`` fields are added. 

243 """ 

244 

245 ConfigClass = ForcedMeasurementConfig 

246 

247 def __init__(self, refSchema, algMetadata=None, **kwds): 

248 super(ForcedMeasurementTask, self).__init__(algMetadata=algMetadata, **kwds) 

249 self.mapper = lsst.afw.table.SchemaMapper(refSchema) 

250 self.mapper.addMinimalSchema(lsst.afw.table.SourceTable.makeMinimalSchema(), False) 

251 self.config.slots.setupSchema(self.mapper.editOutputSchema()) 

252 for refName, targetName in self.config.copyColumns.items(): 

253 refItem = refSchema.find(refName) 

254 self.mapper.addMapping(refItem.key, targetName) 

255 self.config.slots.setupSchema(self.mapper.editOutputSchema()) 

256 self.initializePlugins(schemaMapper=self.mapper) 

257 self.addInvalidPsfFlag(self.mapper.editOutputSchema()) 

258 self.schema = self.mapper.getOutputSchema() 

259 self.schema.checkUnits(parse_strict=self.config.checkUnitsParseStrict) 

260 

261 def run( 

262 self, 

263 measCat, 

264 exposure, 

265 refCat, 

266 refWcs, 

267 exposureId=None, 

268 beginOrder=None, 

269 endOrder=None, 

270 ): 

271 r"""Perform forced measurement. 

272 

273 Parameters 

274 ---------- 

275 exposure : `lsst.afw.image.exposureF` 

276 Image to be measured. Must have at least a `lsst.afw.geom.SkyWcs` 

277 attached. 

278 measCat : `lsst.afw.table.SourceCatalog` 

279 Source catalog for measurement results; must be initialized with 

280 empty records already corresponding to those in ``refCat`` (via 

281 e.g. `generateMeasCat`). 

282 refCat : `lsst.afw.table.SourceCatalog` 

283 A sequence of `lsst.afw.table.SourceRecord` objects that provide 

284 reference information for the measurement. These will be passed 

285 to each plugin in addition to the output 

286 `~lsst.afw.table.SourceRecord`. 

287 refWcs : `lsst.afw.geom.SkyWcs` 

288 Defines the X,Y coordinate system of ``refCat``. 

289 exposureId : `int`, optional 

290 Optional unique exposureId used to calculate random number 

291 generator seed in the NoiseReplacer. 

292 beginOrder : `int`, optional 

293 Beginning execution order (inclusive). Algorithms with 

294 ``executionOrder`` < ``beginOrder`` are not executed. `None` for no limit. 

295 endOrder : `int`, optional 

296 Ending execution order (exclusive). Algorithms with 

297 ``executionOrder`` >= ``endOrder`` are not executed. `None` for no limit. 

298 

299 Notes 

300 ----- 

301 Fills the initial empty `~lsst.afw.table.SourceCatalog` with forced 

302 measurement results. Two steps must occur before `run` can be called: 

303 

304 - `generateMeasCat` must be called to create the output ``measCat`` 

305 argument. 

306 - `~lsst.afw.detection.Footprint`\ s appropriate for the forced sources 

307 must be attached to the ``measCat`` records. The 

308 `attachTransformedFootprints` method can be used to do this, but 

309 this degrades "heavy" (i.e., including pixel values) 

310 `~lsst.afw.detection.Footprint`\s to regular 

311 `~lsst.afw.detection.Footprint`\s, leading to non-deblended 

312 measurement, so most callers should provide 

313 `~lsst.afw.detection.Footprint`\s some other way. Typically, calling 

314 code will have access to information that will allow them to provide 

315 heavy footprints - for instance, `ForcedPhotCoaddTask` uses the 

316 heavy footprints from deblending run in the same band just before 

317 non-forced is run measurement in that band. 

318 """ 

319 # Construct a footprints dict which looks like 

320 # {ref.getId(): (ref.getParent(), source.getFootprint())} 

321 # (i.e. getting the footprint from the transformed source footprint) 

322 footprints = {ref.getId(): (ref.getParent(), measRecord.getFootprint()) 

323 for (ref, measRecord) in zip(refCat, measCat)} 

324 

325 self.log.info("Performing forced measurement on %d source%s", len(refCat), 

326 "" if len(refCat) == 1 else "s") 

327 

328 # Wrap the task logger into a periodic logger. 

329 periodicLog = PeriodicLogger(self.log) 

330 

331 # Initialize the noise replacer 

332 noiseReplacer = self.initNoiseReplacer(exposure, measCat, footprints, exposureId) 

333 

334 for recordIndex, (measRecord, refRecord) in enumerate(zip(measCat, refCat)): 

335 # Insert source into noise replacer 

336 noiseReplacer.insertSource(refRecord.getId()) 

337 self.callMeasure(measRecord, exposure, refRecord, refWcs, 

338 beginOrder=beginOrder, endOrder=endOrder) 

339 noiseReplacer.removeSource(refRecord.getId()) 

340 periodicLog.log("Forced measurement complete for %d sources out of %d", 

341 recordIndex + 1, len(refCat)) 

342 

343 # When done, restore the exposure to its original state 

344 noiseReplacer.end() 

345 

346 # Undeblended plugins only fire if we're running everything 

347 if endOrder is None: 

348 for recordIndex, (measRecord, refRecord) in enumerate(zip(measCat, refCat)): 

349 for plugin in self.undeblendedPlugins.iter(): 

350 self.doMeasurement(plugin, measRecord, exposure, refRecord, refWcs) 

351 periodicLog.log("Undeblended forced measurement complete for %d sources out of %d", 

352 recordIndex + 1, len(refCat)) 

353 

354 def generateMeasCat(self, exposure, refCat, refWcs, idFactory=None): 

355 r"""Initialize an output catalog from the reference catalog. 

356 

357 Parameters 

358 ---------- 

359 exposure : `lsst.afw.image.exposureF` 

360 Image to be measured. 

361 refCat : iterable of `lsst.afw.table.SourceRecord` 

362 Catalog of reference sources. 

363 refWcs : `lsst.afw.geom.SkyWcs` 

364 Defines the X,Y coordinate system of ``refCat``. 

365 This parameter is not currently used. 

366 idFactory : `lsst.afw.table.IdFactory`, optional 

367 Factory for creating IDs for sources. 

368 

369 Returns 

370 ------- 

371 meascat : `lsst.afw.table.SourceCatalog` 

372 Source catalog ready for measurement. 

373 

374 Notes 

375 ----- 

376 This generates a new blank `~lsst.afw.table.SourceRecord` for each 

377 record in ``refCat``. Note that this method does not attach any 

378 `~lsst.afw.detection.Footprint`\ s. Doing so is up to the caller (who 

379 may call `attachedTransformedFootprints` or define their own method - 

380 see `run` for more information). 

381 """ 

382 if idFactory is None: 

383 idFactory = lsst.afw.table.IdFactory.makeSimple() 

384 table = lsst.afw.table.SourceTable.make(self.schema, idFactory) 

385 measCat = lsst.afw.table.SourceCatalog(table) 

386 table = measCat.table 

387 table.setMetadata(self.algMetadata) 

388 table.preallocate(len(refCat)) 

389 for ref in refCat: 

390 newSource = measCat.addNew() 

391 newSource.assign(ref, self.mapper) 

392 return measCat 

393 

394 def attachTransformedFootprints(self, sources, refCat, exposure, refWcs): 

395 r"""Attach Footprints to blank sources prior to measurement, by 

396 transforming Footprints attached to the reference catalog. 

397 

398 Notes 

399 ----- 

400 `~lsst.afw.detection.Footprint`\s for forced photometry must be in the 

401 pixel coordinate system of the image being measured, while the actual 

402 detections may start out in a different coordinate system. This 

403 default implementation transforms the Footprints from the reference 

404 catalog from the WCS to the exposure's WCS, which downgrades 

405 ``HeavyFootprint``\s into regular `~lsst.afw.detection.Footprint`\s, 

406 destroying deblend information. 

407 

408 See the documentation for `run` for information about the 

409 relationships between `run`, `generateMeasCat`, and 

410 `attachTransformedFootprints`. 

411 """ 

412 exposureWcs = exposure.getWcs() 

413 region = exposure.getBBox(lsst.afw.image.PARENT) 

414 for srcRecord, refRecord in zip(sources, refCat): 

415 srcRecord.setFootprint(refRecord.getFootprint().transform(refWcs, exposureWcs, region)) 

416 

417 def attachPsfShapeFootprints(self, sources, exposure, scaling=3): 

418 """Attach Footprints to blank sources prior to measurement, by 

419 creating elliptical Footprints from the PSF moments. 

420 

421 Parameters 

422 ---------- 

423 sources : `lsst.afw.table.SourceCatalog` 

424 Blank catalog (with all rows and columns, but values other than 

425 ``coord_ra``, ``coord_dec`` unpopulated). 

426 to which footprints should be attached. 

427 exposure : `lsst.afw.image.Exposure` 

428 Image object from which peak values and the PSF are obtained. 

429 scaling : `int`, optional 

430 Scaling factor to apply to the PSF second-moments ellipse in order 

431 to determine the footprint boundary. 

432 

433 Notes 

434 ----- 

435 This is a utility function for use by parent tasks; see 

436 `attachTransformedFootprints` for more information. 

437 """ 

438 psf = exposure.getPsf() 

439 if psf is None: 

440 raise RuntimeError("Cannot construct Footprints from PSF shape without a PSF.") 

441 bbox = exposure.getBBox() 

442 wcs = exposure.getWcs() 

443 for record in sources: 

444 localPoint = wcs.skyToPixel(record.getCoord()) 

445 localIntPoint = lsst.geom.Point2I(localPoint) 

446 assert bbox.contains(localIntPoint), ( 

447 f"Center for record {record.getId()} is not in exposure; this should be guaranteed by " 

448 "generateMeasCat." 

449 ) 

450 ellipse = lsst.afw.geom.ellipses.Ellipse(psf.computeShape(localPoint), localPoint) 

451 ellipse.getCore().scale(scaling) 

452 spans = lsst.afw.geom.SpanSet.fromShape(ellipse) 

453 footprint = lsst.afw.detection.Footprint(spans.clippedTo(bbox), bbox) 

454 footprint.addPeak(localIntPoint.getX(), localIntPoint.getY(), 

455 exposure.image._get(localIntPoint, lsst.afw.image.PARENT)) 

456 record.setFootprint(footprint)