22 r"""Base classes for forced measurement plugins and the driver task for these.
24 In forced measurement, a reference catalog is used to define restricted
25 measurements (usually just fluxes) on an image. As the reference catalog may
26 be deeper than the detection limit of the measurement image, we do not assume
27 that we can use detection and deblend information from the measurement image.
28 Instead, we assume this information is present in the reference catalog and
29 can be "transformed" in some sense to the measurement frame. At the very
30 least, this means that `~lsst.afw.detection.Footprint`\ s from the reference
31 catalog should be transformed and installed as Footprints in the output
32 measurement catalog. If we have a procedure that can transform "heavy"
33 Footprints (ie, including pixel data), we can then proceed with measurement as
34 usual, but using the reference catalog's ``id`` and ``parent`` fields to
35 define deblend families. If this transformation does not preserve
36 heavy Footprints (this is currently the case, at least for CCD forced
37 photometry), then we will only be able to replace objects with noise one
38 deblend family at a time, and hence measurements run in single-object mode may
39 be contaminated by neighbors when run on objects with ``parent != 0``.
41 Measurements are generally recorded in the coordinate system of the image
42 being measured (and all slot-eligible fields must be), but non-slot fields may
43 be recorded in other coordinate systems if necessary to avoid information loss
44 (this should, of course, be indicated in the field documentation). Note that
45 the reference catalog may be in a different coordinate system; it is the
46 responsibility of plugins to transform the data they need themselves, using
47 the reference WCS provided. However, for plugins that only require a position
48 or shape, they may simply use output `~lsst.afw.table.SourceCatalog`\'s
49 centroid or shape slots, which will generally be set to the transformed
50 position of the reference object before any other plugins are run, and hence
51 avoid using the reference catalog at all.
53 Command-line driver tasks for forced measurement include
54 `ForcedPhotImageTask`, `ForcedPhotCcdTask`, and `ForcedPhotCoaddTask`.
60 from .pluginRegistry
import PluginRegistry
61 from .baseMeasurement
import (BaseMeasurementPluginConfig, BaseMeasurementPlugin,
62 BaseMeasurementConfig, BaseMeasurementTask)
63 from .noiseReplacer
import NoiseReplacer, DummyNoiseReplacer
65 __all__ = (
"ForcedPluginConfig",
"ForcedPlugin",
66 "ForcedMeasurementConfig",
"ForcedMeasurementTask")
70 """Base class for configs of forced measurement plugins."""
76 """Base class for forced measurement plugins.
80 config : `ForcedPlugin.ConfigClass`
81 Configuration for this plugin.
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.
96 """Subclasses of `ForcedPlugin` must be registered here (`PluginRegistry`).
99 ConfigClass = ForcedPluginConfig
101 def __init__(self, config, name, schemaMapper, metadata, logName=None):
102 BaseMeasurementPlugin.__init__(self, config, name, logName=logName)
104 def measure(self, measRecord, exposure, refRecord, refWcs):
105 """Measure the properties of a source given an image and a reference.
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
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.
132 raise NotImplementedError()
134 def measureN(self, measCat, exposure, refCat, refWcs):
135 """Measure the properties of blended sources from image & reference.
137 This operates on all members of a blend family at once.
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
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
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.
166 raise NotImplementedError()
170 """Config class for forced measurement driver task.
173 plugins = ForcedPlugin.registry.makeField(
175 default=[
"base_PixelFlags",
176 "base_TransformedCentroid",
178 "base_TransformedShape",
181 "base_CircularApertureFlux",
183 "base_LocalBackground",
185 doc=
"Plugins to be run and their configuration"
187 algorithms = property(
lambda self: self.
plugins, doc=
"backwards-compatibility alias for plugins")
188 undeblended = ForcedPlugin.registry.makeField(
191 doc=
"Plugins to run on undeblended image"
195 keytype=str, itemtype=str, doc=
"Mapping of reference columns to source columns",
196 default={
"id":
"objectId",
"parent":
"parentObjectId",
"deblend_nChild":
"deblend_nChild",
197 "coord_ra":
"coord_ra",
"coord_dec":
"coord_dec"}
201 doc=
"Strictness of Astropy unit compatibility check, can be 'raise', 'warn' or 'silent'",
207 self.
slots.centroid =
"base_TransformedCentroid"
208 self.
slots.shape =
"base_TransformedShape"
209 self.
slots.apFlux =
None
210 self.
slots.modelFlux =
None
211 self.
slots.psfFlux =
None
212 self.
slots.gaussianFlux =
None
213 self.
slots.calibFlux =
None
217 """Measure sources on an image, constrained by a reference catalog.
219 A subtask for measuring the properties of sources on a single image,
220 using an existing "reference" catalog to constrain some aspects of the
225 refSchema : `lsst.afw.table.Schema`
226 Schema of the reference catalog. Must match the catalog later passed
227 to 'ForcedMeasurementTask.generateMeasCat` and/or
228 `ForcedMeasurementTask.run`.
229 algMetadata : `lsst.daf.base.PropertyList` or `None`
230 Will be updated in place to to record information about each
231 algorithm. An empty `~lsst.daf.base.PropertyList` will be created if
234 Keyword arguments are passed to the supertask constructor.
238 Note that while `SingleFrameMeasurementTask` is passed an initial
239 `~lsst.afw.table.Schema` that is appended to in order to create the output
240 `~lsst.afw.table.Schema`, `ForcedMeasurementTask` is initialized with the
241 `~lsst.afw.table.Schema` of the reference catalog, from which a new
242 `~lsst.afw.table.Schema` for the output catalog is created. Fields to be
243 copied directly from the reference `~lsst.afw.table.Schema` are added
244 before ``Plugin`` fields are added.
247 ConfigClass = ForcedMeasurementConfig
249 def __init__(self, refSchema, algMetadata=None, **kwds):
250 super(ForcedMeasurementTask, self).
__init__(algMetadata=algMetadata, **kwds)
253 self.
config.slots.setupSchema(self.
mapper.editOutputSchema())
254 for refName, targetName
in self.
config.copyColumns.items():
255 refItem = refSchema.find(refName)
256 self.
mapper.addMapping(refItem.key, targetName)
257 self.
config.slots.setupSchema(self.
mapper.editOutputSchema())
260 self.
schema.checkUnits(parse_strict=self.
config.checkUnitsParseStrict)
262 def run(self, measCat, exposure, refCat, refWcs, exposureId=None, beginOrder=None, endOrder=None):
263 r"""Perform forced measurement.
267 exposure : `lsst.afw.image.exposureF`
268 Image to be measured. Must have at least a `lsst.afw.geom.SkyWcs`
270 measCat : `lsst.afw.table.SourceCatalog`
271 Source catalog for measurement results; must be initialized with
272 empty records already corresponding to those in ``refCat`` (via
273 e.g. `generateMeasCat`).
274 refCat : `lsst.afw.table.SourceCatalog`
275 A sequence of `lsst.afw.table.SourceRecord` objects that provide
276 reference information for the measurement. These will be passed
277 to each plugin in addition to the output
278 `~lsst.afw.table.SourceRecord`.
279 refWcs : `lsst.afw.geom.SkyWcs`
280 Defines the X,Y coordinate system of ``refCat``.
281 exposureId : `int`, optional
282 Optional unique exposureId used to calculate random number
283 generator seed in the NoiseReplacer.
284 beginOrder : `int`, optional
285 Beginning execution order (inclusive). Algorithms with
286 ``executionOrder`` < ``beginOrder`` are not executed. `None` for no limit.
287 endOrder : `int`, optional
288 Ending execution order (exclusive). Algorithms with
289 ``executionOrder`` >= ``endOrder`` are not executed. `None` for no limit.
293 Fills the initial empty `~lsst.afw.table.SourceCatalog` with forced
294 measurement results. Two steps must occur before `run` can be called:
296 - `generateMeasCat` must be called to create the output ``measCat``
298 - `~lsst.afw.detection.Footprint`\ s appropriate for the forced sources
299 must be attached to the ``measCat`` records. The
300 `attachTransformedFootprints` method can be used to do this, but
301 this degrades "heavy" (i.e., including pixel values)
302 `~lsst.afw.detection.Footprint`\s to regular
303 `~lsst.afw.detection.Footprint`\s, leading to non-deblended
304 measurement, so most callers should provide
305 `~lsst.afw.detection.Footprint`\s some other way. Typically, calling
306 code will have access to information that will allow them to provide
307 heavy footprints - for instance, `ForcedPhotCoaddTask` uses the
308 heavy footprints from deblending run in the same band just before
309 non-forced is run measurement in that band.
321 refCatIdDict = {ref.getId(): ref.getParent()
for ref
in refCat}
326 if topId
not in refCatIdDict:
327 raise RuntimeError(
"Reference catalog contains a child for which at least "
328 "one parent in its parent chain is not in the catalog.")
329 topId = refCatIdDict[topId]
334 footprints = {ref.getId(): (ref.getParent(), measRecord.getFootprint())
335 for (ref, measRecord)
in zip(refCat, measCat)}
337 self.
log.
info(
"Performing forced measurement on %d source%s", len(refCat),
338 "" if len(refCat) == 1
else "s")
340 if self.
config.doReplaceWithNoise:
342 footprints, log=self.
log, exposureId=exposureId)
343 algMetadata = measCat.getTable().getMetadata()
344 if algMetadata
is not None:
345 algMetadata.addInt(
"NOISE_SEED_MULTIPLIER", self.
config.noiseReplacer.noiseSeedMultiplier)
346 algMetadata.addString(
"NOISE_SOURCE", self.
config.noiseReplacer.noiseSource)
347 algMetadata.addDouble(
"NOISE_OFFSET", self.
config.noiseReplacer.noiseOffset)
348 if exposureId
is not None:
349 algMetadata.addLong(
"NOISE_EXPOSURE_ID", exposureId)
355 refParentCat, measParentCat = refCat.getChildren(0, measCat)
356 for parentIdx, (refParentRecord, measParentRecord)
in enumerate(zip(refParentCat, measParentCat)):
359 refChildCat, measChildCat = refCat.getChildren(refParentRecord.getId(), measCat)
361 for refChildRecord, measChildRecord
in zip(refChildCat, measChildCat):
362 noiseReplacer.insertSource(refChildRecord.getId())
363 self.
callMeasure(measChildRecord, exposure, refChildRecord, refWcs,
364 beginOrder=beginOrder, endOrder=endOrder)
365 noiseReplacer.removeSource(refChildRecord.getId())
368 noiseReplacer.insertSource(refParentRecord.getId())
369 self.
callMeasure(measParentRecord, exposure, refParentRecord, refWcs,
370 beginOrder=beginOrder, endOrder=endOrder)
371 self.
callMeasureN(measParentCat[parentIdx:parentIdx+1], exposure,
372 refParentCat[parentIdx:parentIdx+1],
373 beginOrder=beginOrder, endOrder=endOrder)
376 beginOrder=beginOrder, endOrder=endOrder)
377 noiseReplacer.removeSource(refParentRecord.getId())
382 for measRecord, refRecord
in zip(measCat, refCat):
384 self.
doMeasurement(plugin, measRecord, exposure, refRecord, refWcs)
387 r"""Initialize an output catalog from the reference catalog.
391 exposure : `lsst.afw.image.exposureF`
392 Image to be measured.
393 refCat : iterable of `lsst.afw.table.SourceRecord`
394 Catalog of reference sources.
395 refWcs : `lsst.afw.geom.SkyWcs`
396 Defines the X,Y coordinate system of ``refCat``.
397 idFactory : `lsst.afw.table.IdFactory`, optional
398 Factory for creating IDs for sources.
402 meascat : `lsst.afw.table.SourceCatalog`
403 Source catalog ready for measurement.
407 This generates a new blank `~lsst.afw.table.SourceRecord` for each
408 record in ``refCat``. Note that this method does not attach any
409 `~lsst.afw.detection.Footprint`\ s. Doing so is up to the caller (who
410 may call `attachedTransformedFootprints` or define their own method -
411 see `run` for more information).
413 if idFactory
is None:
417 table = measCat.table
419 table.preallocate(len(refCat))
421 newSource = measCat.addNew()
422 newSource.assign(ref, self.
mapper)
426 r"""Attach Footprints to blank sources prior to measurement.
430 `~lsst.afw.detection.Footprint`\s for forced photometry must be in the
431 pixel coordinate system of the image being measured, while the actual
432 detections may start out in a different coordinate system. This
433 default implementation transforms the Footprints from the reference
434 catalog from the WCS to the exposure's WCS, which downgrades
435 ``HeavyFootprint``\s into regular `~lsst.afw.detection.Footprint`\s,
436 destroying deblend information.
438 Note that `ForcedPhotImageTask` delegates to this method in its own
439 `~ForcedPhotImageTask.attachFootprints` method. This method can be
440 overridden by its subclasses to define how their
441 `~lsst.afw.detection.Footprint`\s should be generated.
443 See the documentation for `run` for information about the
444 relationships between `run`, `generateMeasCat`, and
445 `attachTransformedFootprints`.
447 exposureWcs = exposure.getWcs()
448 region = exposure.getBBox(lsst.afw.image.PARENT)
449 for srcRecord, refRecord
in zip(sources, refCat):
450 srcRecord.setFootprint(refRecord.getFootprint().
transform(refWcs, exposureWcs, region))