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LSST Data Management Base Package
dipoleMeasurement.py
Go to the documentation of this file.
1# This file is part of ip_diffim.
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/>.
21
22import numpy as np
23
24import lsst.afw.image as afwImage
25import lsst.geom as geom
26import lsst.pex.config as pexConfig
27import lsst.meas.deblender.baseline as deblendBaseline
28from lsst.meas.base.pluginRegistry import register
29from lsst.meas.base import SingleFrameMeasurementTask, SingleFrameMeasurementConfig, \
30 SingleFramePluginConfig, SingleFramePlugin
31import lsst.afw.display as afwDisplay
32from lsst.utils.logging import getLogger
33
34__all__ = ("DipoleMeasurementConfig", "DipoleMeasurementTask", "DipoleAnalysis", "DipoleDeblender",
35 "SourceFlagChecker", "ClassificationDipoleConfig", "ClassificationDipolePlugin")
36
37
39 """Configuration for classification of detected diaSources as dipole or not"""
40 minSn = pexConfig.Field(
41 doc="Minimum quadrature sum of positive+negative lobe S/N to be considered a dipole",
42 dtype=float, default=np.sqrt(2) * 5.0,
43 )
44 maxFluxRatio = pexConfig.Field(
45 doc="Maximum flux ratio in either lobe to be considered a dipole",
46 dtype=float, default=0.65
47 )
48
49
50@register("ip_diffim_ClassificationDipole")
52 """A plugin to classify whether a diaSource is a dipole.
53 """
54
55 ConfigClass = ClassificationDipoleConfig
56
57 @classmethod
59 """
60 Returns
61 -------
62 result : `callable`
63 """
64 return cls.APCORR_ORDERAPCORR_ORDER
65
66 def __init__(self, config, name, schema, metadata):
67 SingleFramePlugin.__init__(self, config, name, schema, metadata)
68 self.dipoleAnalysisdipoleAnalysis = DipoleAnalysis()
69 self.keyProbabilitykeyProbability = schema.addField(name + "_value", type="D",
70 doc="Set to 1 for dipoles, else 0.")
71 self.keyFlagkeyFlag = schema.addField(name + "_flag", type="Flag", doc="Set to 1 for any fatal failure.")
72
73 def measure(self, measRecord, exposure):
74 passesSn = self.dipoleAnalysisdipoleAnalysis.getSn(measRecord) > self.configconfig.minSn
75 negFlux = np.abs(measRecord.get("ip_diffim_PsfDipoleFlux_neg_instFlux"))
76 negFluxFlag = measRecord.get("ip_diffim_PsfDipoleFlux_neg_flag")
77 posFlux = np.abs(measRecord.get("ip_diffim_PsfDipoleFlux_pos_instFlux"))
78 posFluxFlag = measRecord.get("ip_diffim_PsfDipoleFlux_pos_flag")
79
80 if negFluxFlag or posFluxFlag:
81 self.failfailfail(measRecord)
82 # continue on to classify
83
84 totalFlux = negFlux + posFlux
85
86 # If negFlux or posFlux are NaN, these evaluate to False
87 passesFluxNeg = (negFlux / totalFlux) < self.configconfig.maxFluxRatio
88 passesFluxPos = (posFlux / totalFlux) < self.configconfig.maxFluxRatio
89 if (passesSn and passesFluxPos and passesFluxNeg):
90 val = 1.0
91 else:
92 val = 0.0
93
94 measRecord.set(self.keyProbabilitykeyProbability, val)
95
96 def fail(self, measRecord, error=None):
97 measRecord.set(self.keyFlagkeyFlag, True)
98
99
101 """Measurement of detected diaSources as dipoles"""
102
103 def setDefaults(self):
104 SingleFrameMeasurementConfig.setDefaults(self)
105 self.pluginspluginsplugins = ["base_CircularApertureFlux",
106 "base_PixelFlags",
107 "base_SkyCoord",
108 "base_PsfFlux",
109 "ip_diffim_NaiveDipoleCentroid",
110 "ip_diffim_NaiveDipoleFlux",
111 "ip_diffim_PsfDipoleFlux",
112 "ip_diffim_ClassificationDipole",
113 ]
114
115 self.slotsslots.calibFlux = None
116 self.slotsslots.modelFlux = None
117 self.slotsslots.gaussianFlux = None
118 self.slotsslots.shape = None
119 self.slotsslots.centroid = "ip_diffim_NaiveDipoleCentroid"
120 self.doReplaceWithNoisedoReplaceWithNoisedoReplaceWithNoise = False
121
122
124 """Measurement of Sources, specifically ones from difference images, for characterization as dipoles
125
126 Parameters
127 ----------
128 sources : 'lsst.afw.table.SourceCatalog'
129 Sources that will be measured
130 badFlags : `list` of `dict`
131 A list of flags that will be used to determine if there was a measurement problem
132
133 Notes
134 -----
135 The list of badFlags will be used to make a list of keys to check for measurement flags on. By
136 default the centroid keys are added to this list
137
138 Description
139
140 This class provides a default configuration for running Source measurement on image differences.
141
142 .. code-block:: py
143
145 "Measurement of detected diaSources as dipoles"
146 def setDefaults(self):
147 SingleFrameMeasurementConfig.setDefaults(self)
148 self.pluginsplugins = ["base_CircularApertureFlux",
149 "base_PixelFlags",
150 "base_SkyCoord",
151 "base_PsfFlux",
152 "ip_diffim_NaiveDipoleCentroid",
153 "ip_diffim_NaiveDipoleFlux",
154 "ip_diffim_PsfDipoleFlux",
155 "ip_diffim_ClassificationDipole",
156 ]
157 self.slots.calibFlux = None
158 self.slots.modelFlux = None
159 self.slots.instFlux = None
160 self.slots.shape = None
161 self.slots.centroid = "ip_diffim_NaiveDipoleCentroid"
162 self.doReplaceWithNoise = False
163
164 These plugins enabled by default allow the user to test the hypothesis that the Source is a dipole.
165 This includes a set of measurements derived from intermediate base classes
166 DipoleCentroidAlgorithm and DipoleFluxAlgorithm.
167 Their respective algorithm control classes are defined in
168 DipoleCentroidControl and DipoleFluxControl.
169 Each centroid and flux measurement will have _neg (negative)
170 and _pos (positive lobe) fields.
171
172 The first set of measurements uses a "naive" alrogithm
173 for centroid and flux measurements, implemented in
174 NaiveDipoleCentroidControl and NaiveDipoleFluxControl.
175 The algorithm uses a naive 3x3 weighted moment around
176 the nominal centroids of each peak in the Source Footprint. These algorithms fill the table fields
177 ip_diffim_NaiveDipoleCentroid* and ip_diffim_NaiveDipoleFlux*
178
179 The second set of measurements undertakes a joint-Psf model on the negative
180 and positive lobe simultaneously. This fit simultaneously solves for the negative and positive
181 lobe centroids and fluxes using non-linear least squares minimization.
182 The fields are stored in table elements ip_diffim_PsfDipoleFlux*.
183
184 Because this Task is just a config for SingleFrameMeasurementTask, the same result may be acheived by
185 manually editing the config and running SingleFrameMeasurementTask. For example:
186
187 .. code-block:: py
188
190 config.plugins.names = ["base_PsfFlux",
191 "ip_diffim_PsfDipoleFlux",
192 "ip_diffim_NaiveDipoleFlux",
193 "ip_diffim_NaiveDipoleCentroid",
194 "ip_diffim_ClassificationDipole",
195 "base_CircularApertureFlux",
196 "base_SkyCoord"]
197
198 config.slots.calibFlux = None
199 config.slots.modelFlux = None
200 config.slots.instFlux = None
201 config.slots.shape = None
202 config.slots.centroid = "ip_diffim_NaiveDipoleCentroid"
203 config.doReplaceWithNoise = False
204
205 schema = afwTable.SourceTable.makeMinimalSchema()
206 task = SingleFrameMeasurementTask(schema, config=config)-
207
208 Debug variables
209
210 The ``lsst.pipe.base.cmdLineTask.CmdLineTask`` command line task interface supports a
211 flag-d/--debug to import debug.py from your PYTHONPATH. The relevant contents of debug.py
212 for this Task include:
213
214 .. code-block:: py
215
216 import sys
217 import lsstDebug
218 def DebugInfo(name):
219 di = lsstDebug.getInfo(name)
220 if name == "lsst.ip.diffim.dipoleMeasurement":
221 di.display = True # enable debug output
222 di.maskTransparency = 90 # display mask transparency
223 di.displayDiaSources = True # show exposure with dipole results
224 return di
225 lsstDebug.Info = DebugInfo
226 lsstDebug.frame = 1
227
228 config.slots.calibFlux = None
229 config.slots.modelFlux = None
230 config.slots.gaussianFlux = None
231 config.slots.shape = None
232 config.slots.centroid = "ip_diffim_NaiveDipoleCentroid"
233 config.doReplaceWithNoise = False
234
235 This code is dipoleMeasTask.py in the examples directory, and can be run as e.g.
236
237 .. code-block:: none
238
239 examples/dipoleMeasTask.py
240 examples/dipoleMeasTask.py --debug
241 examples/dipoleMeasTask.py --debug --image /path/to/image.fits
242
243
244
245 Start the processing by parsing the command line, where the user has the option of
246 enabling debugging output and/or sending their own image for demonstration
247 (in case they have not downloaded the afwdata package).
248
249 .. code-block:: py
250
251 if __name__ == "__main__":
252 import argparse
253 parser = argparse.ArgumentParser(
254 description="Demonstrate the use of SourceDetectionTask and DipoleMeasurementTask")
255 parser.add_argument('--debug', '-d', action="store_true", help="Load debug.py?", default=False)
256 parser.add_argument("--image", "-i", help="User defined image", default=None)
257 args = parser.parse_args()
258 if args.debug:
259 try:
260 import debug
261 debug.lsstDebug.frame = 2
262 except ImportError as e:
263 print(e, file=sys.stderr)
264 run(args)
265
266 The processing occurs in the run function. We first extract an exposure from disk or afwdata, displaying
267 it if requested:
268
269 .. code-block:: py
270
271 def run(args):
272 exposure = loadData(args.image)
273 if args.debug:
274 afwDisplay.Display(frame=1).mtv(exposure)
275
276 Create a default source schema that we will append fields to as we add more algorithms:
277
278 .. code-block:: py
279
280 schema = afwTable.SourceTable.makeMinimalSchema()
281
282 Create the detection and measurement Tasks, with some minor tweaking of their configs:
283
284 .. code-block:: py
285
286 # Create the detection task
287 config = SourceDetectionTask.ConfigClass()
288 config.thresholdPolarity = "both"
289 config.background.isNanSafe = True
290 config.thresholdValue = 3
291 detectionTask = SourceDetectionTask(config=config, schema=schema)
292 # And the measurement Task
293 config = DipoleMeasurementTask.ConfigClass()
294 config.plugins.names.remove('base_SkyCoord')
295 algMetadata = dafBase.PropertyList()
296 measureTask = DipoleMeasurementTask(schema, algMetadata, config=config)
297
298 Having fully initialied the schema, we create a Source table from it:
299
300 .. code-block:: py
301
302 # Create the output table
303 tab = afwTable.SourceTable.make(schema)
304
305 Run detection:
306
307 .. code-block:: py
308
309 # Process the data
310 results = detectionTask.run(tab, exposure)
311
312 Because we are looking for dipoles, we need to merge the positive and negative detections:
313
314 .. code-block:: py
315
316 # Merge the positve and negative sources
317 fpSet = results.fpSets.positive
318 growFootprint = 2
319 fpSet.merge(results.fpSets.negative, growFootprint, growFootprint, False)
320 diaSources = afwTable.SourceCatalog(tab)
321 fpSet.makeSources(diaSources)
322 print("Merged %s Sources into %d diaSources (from %d +ve, %d -ve)" % (len(results.sources),
323 len(diaSources),
324 results.fpSets.numPos,
325 results.fpSets.numNeg))
326
327 Finally, perform measurement (both standard and dipole-specialized) on the merged sources:
328
329 .. code-block:: py
330
331 measureTask.run(diaSources, exposure)
332
333 Optionally display debugging information:
334
335 .. code-block:: py
336
337 # Display dipoles if debug enabled
338 if args.debug:
339 dpa = DipoleAnalysis()
340 dpa.displayDipoles(exposure, diaSources)
341
342 """
343 ConfigClass = DipoleMeasurementConfig
344 _DefaultName = "dipoleMeasurement"
345
346
347
350
352 """Functor class to check whether a diaSource has flags set that should cause it to be labeled bad."""
353
354 def __init__(self, sources, badFlags=None):
355 self.badFlagsbadFlags = ['base_PixelFlags_flag_edge', 'base_PixelFlags_flag_interpolatedCenter',
356 'base_PixelFlags_flag_saturatedCenter']
357 if badFlags is not None:
358 for flag in badFlags:
359 self.badFlagsbadFlags.append(flag)
360 self.keyskeys = [sources.getSchema().find(name).key for name in self.badFlagsbadFlags]
361 self.keyskeys.append(sources.table.getCentroidFlagKey())
362
363 def __call__(self, source):
364 """Call the source flag checker on a single Source
365
366 Parameters
367 ----------
368 source :
369 Source that will be examined
370 """
371 for k in self.keyskeys:
372 if source.get(k):
373 return False
374 return True
375
376
378 """Functor class that provides (S/N, position, orientation) of measured dipoles"""
379
380 def __init__(self):
381 pass
382
383 def __call__(self, source):
384 """Parse information returned from dipole measurement
385
386 Parameters
387 ----------
389 The source that will be examined"""
390 return self.getSn(source), self.getCentroid(source), self.getOrientation(source)
391
392 def getSn(self, source):
393 """Get the total signal-to-noise of the dipole; total S/N is from positive and negative lobe
394
395 Parameters
396 ----------
398 The source that will be examined"""
399
400 posflux = source.get("ip_diffim_PsfDipoleFlux_pos_instFlux")
401 posfluxErr = source.get("ip_diffim_PsfDipoleFlux_pos_instFluxErr")
402 negflux = source.get("ip_diffim_PsfDipoleFlux_neg_instFlux")
403 negfluxErr = source.get("ip_diffim_PsfDipoleFlux_neg_instFluxErr")
404
405 # Not a dipole!
406 if (posflux < 0) is (negflux < 0):
407 return 0
408
409 return np.sqrt((posflux/posfluxErr)**2 + (negflux/negfluxErr)**2)
410
411 def getCentroid(self, source):
412 """Get the centroid of the dipole; average of positive and negative lobe
413
414 Parameters
415 ----------
417 The source that will be examined"""
418
419 negCenX = source.get("ip_diffim_PsfDipoleFlux_neg_centroid_x")
420 negCenY = source.get("ip_diffim_PsfDipoleFlux_neg_centroid_y")
421 posCenX = source.get("ip_diffim_PsfDipoleFlux_pos_centroid_x")
422 posCenY = source.get("ip_diffim_PsfDipoleFlux_pos_centroid_y")
423 if (np.isinf(negCenX) or np.isinf(negCenY) or np.isinf(posCenX) or np.isinf(posCenY)):
424 return None
425
426 center = geom.Point2D(0.5*(negCenX+posCenX),
427 0.5*(negCenY+posCenY))
428 return center
429
430 def getOrientation(self, source):
431 """Calculate the orientation of dipole; vector from negative to positive lobe
432
433 Parameters
434 ----------
436 The source that will be examined"""
437
438 negCenX = source.get("ip_diffim_PsfDipoleFlux_neg_centroid_x")
439 negCenY = source.get("ip_diffim_PsfDipoleFlux_neg_centroid_y")
440 posCenX = source.get("ip_diffim_PsfDipoleFlux_pos_centroid_x")
441 posCenY = source.get("ip_diffim_PsfDipoleFlux_pos_centroid_y")
442 if (np.isinf(negCenX) or np.isinf(negCenY) or np.isinf(posCenX) or np.isinf(posCenY)):
443 return None
444
445 dx, dy = posCenX-negCenX, posCenY-negCenY
446 angle = geom.Angle(np.arctan2(dx, dy), geom.radians)
447 return angle
448
449 def displayDipoles(self, exposure, sources):
450 """Display debugging information on the detected dipoles
451
452 Parameters
453 ----------
454 exposure : `lsst.afw.image.Exposure`
455 Image the dipoles were measured on
457 The set of diaSources that were measured"""
458
459 import lsstDebug
460 display = lsstDebug.Info(__name__).display
461 displayDiaSources = lsstDebug.Info(__name__).displayDiaSources
462 maskTransparency = lsstDebug.Info(__name__).maskTransparency
463 if not maskTransparency:
464 maskTransparency = 90
465 disp = afwDisplay.Display(frame=lsstDebug.frame)
466 disp.setMaskTransparency(maskTransparency)
467 disp.mtv(exposure)
468
469 if display and displayDiaSources:
470 with disp.Buffering():
471 for source in sources:
472 cenX, cenY = source.get("ipdiffim_DipolePsfFlux_centroid")
473 if np.isinf(cenX) or np.isinf(cenY):
474 cenX, cenY = source.getCentroid()
475
476 isdipole = source.get("ip_diffim_ClassificationDipole_value")
477 if isdipole and np.isfinite(isdipole):
478 # Dipole
479 ctype = afwDisplay.GREEN
480 else:
481 # Not dipole
482 ctype = afwDisplay.RED
483
484 disp.dot("o", cenX, cenY, size=2, ctype=ctype)
485
486 negCenX = source.get("ip_diffim_PsfDipoleFlux_neg_centroid_x")
487 negCenY = source.get("ip_diffim_PsfDipoleFlux_neg_centroid_y")
488 posCenX = source.get("ip_diffim_PsfDipoleFlux_pos_centroid_x")
489 posCenY = source.get("ip_diffim_PsfDipoleFlux_pos_centroid_y")
490 if (np.isinf(negCenX) or np.isinf(negCenY) or np.isinf(posCenX) or np.isinf(posCenY)):
491 continue
492
493 disp.line([(negCenX, negCenY), (posCenX, posCenY)], ctype=afwDisplay.YELLOW)
494
495 lsstDebug.frame += 1
496
497
499 """Functor to deblend a source as a dipole, and return a new source with deblended footprints.
500
501 This necessarily overrides some of the functionality from
502 meas_algorithms/python/lsst/meas/algorithms/deblend.py since we
503 need a single source that contains the blended peaks, not
504 multiple children sources. This directly calls the core
505 deblending code deblendBaseline.deblend (optionally _fitPsf for
506 debugging).
507
508 Not actively being used, but there is a unit test for it in
509 dipoleAlgorithm.py.
510 """
511
512 def __init__(self):
513 # Set up defaults to send to deblender
514
515 # Always deblend as Psf
516 self.psfChisqCut1psfChisqCut1 = self.psfChisqCut2psfChisqCut2 = self.psfChisqCut2bpsfChisqCut2b = np.inf
517 self.loglog = getLogger('lsst.ip.diffim.DipoleDeblender')
518 self.sigma2fwhmsigma2fwhm = 2. * np.sqrt(2. * np.log(2.))
519
520 def __call__(self, source, exposure):
521 fp = source.getFootprint()
522 peaks = fp.getPeaks()
523 peaksF = [pk.getF() for pk in peaks]
524 fbb = fp.getBBox()
525 fmask = afwImage.Mask(fbb)
526 fmask.setXY0(fbb.getMinX(), fbb.getMinY())
527 fp.spans.setMask(fmask, 1)
528
529 psf = exposure.getPsf()
530 psfSigPix = psf.computeShape(psf.getAveragePosition()).getDeterminantRadius()
531 psfFwhmPix = psfSigPix * self.sigma2fwhmsigma2fwhm
532 subimage = afwImage.ExposureF(exposure, bbox=fbb, deep=True)
533 cpsf = deblendBaseline.CachingPsf(psf)
534
535 # if fewer than 2 peaks, just return a copy of the source
536 if len(peaks) < 2:
537 return source.getTable().copyRecord(source)
538
539 # make sure you only deblend 2 peaks; take the brighest and faintest
540 speaks = [(p.getPeakValue(), p) for p in peaks]
541 speaks.sort()
542 dpeaks = [speaks[0][1], speaks[-1][1]]
543
544 # and only set these peaks in the footprint (peaks is mutable)
545 peaks.clear()
546 for peak in dpeaks:
547 peaks.append(peak)
548
549 if True:
550 # Call top-level deblend task
551 fpres = deblendBaseline.deblend(fp, exposure.getMaskedImage(), psf, psfFwhmPix,
552 log=self.loglog,
553 psfChisqCut1=self.psfChisqCut1psfChisqCut1,
554 psfChisqCut2=self.psfChisqCut2psfChisqCut2,
555 psfChisqCut2b=self.psfChisqCut2bpsfChisqCut2b)
556 else:
557 # Call lower-level _fit_psf task
558
559 # Prepare results structure
560 fpres = deblendBaseline.DeblenderResult(fp, exposure.getMaskedImage(), psf, psfFwhmPix, self.loglog)
561
562 for pki, (pk, pkres, pkF) in enumerate(zip(dpeaks, fpres.deblendedParents[0].peaks, peaksF)):
563 self.loglog.debug('Peak %i', pki)
564 deblendBaseline._fitPsf(fp, fmask, pk, pkF, pkres, fbb, dpeaks, peaksF, self.loglog,
565 cpsf, psfFwhmPix,
566 subimage.getMaskedImage().getImage(),
567 subimage.getMaskedImage().getVariance(),
568 self.psfChisqCut1psfChisqCut1, self.psfChisqCut2psfChisqCut2, self.psfChisqCut2bpsfChisqCut2b)
569
570 deblendedSource = source.getTable().copyRecord(source)
571 deblendedSource.setParent(source.getId())
572 peakList = deblendedSource.getFootprint().getPeaks()
573 peakList.clear()
574
575 for i, peak in enumerate(fpres.deblendedParents[0].peaks):
576 if peak.psfFitFlux > 0:
577 suffix = "pos"
578 else:
579 suffix = "neg"
580 c = peak.psfFitCenter
581 self.loglog.info("deblended.centroid.dipole.psf.%s %f %f",
582 suffix, c[0], c[1])
583 self.loglog.info("deblended.chi2dof.dipole.%s %f",
584 suffix, peak.psfFitChisq / peak.psfFitDof)
585 self.loglog.info("deblended.flux.dipole.psf.%s %f",
586 suffix, peak.psfFitFlux * np.sum(peak.templateImage.getArray()))
587 peakList.append(peak.peak)
588 return deblendedSource
table::Key< int > a
A class to contain the data, WCS, and other information needed to describe an image of the sky.
Definition: Exposure.h:72
Represent a 2-dimensional array of bitmask pixels.
Definition: Mask.h:77
Record class that contains measurements made on a single exposure.
Definition: Source.h:78
Class for storing ordered metadata with comments.
Definition: PropertyList.h:68
A class representing an angle.
Definition: Angle.h:128
def __init__(self, config, name, schema, metadata)
def fail(self, measRecord, error=None)
Definition: pluginsBase.py:137
def run(self, measCat, exposure, noiseImage=None, exposureId=None, beginOrder=None, endOrder=None)
Definition: sfm.py:215
std::shared_ptr< FrameSet > append(FrameSet const &first, FrameSet const &second)
Construct a FrameSet that performs two transformations in series.
Definition: functional.cc:33
def mtv(data, frame=None, title="", wcs=None, *args, **kwargs)
Definition: ds9.py:92
Backwards-compatibility support for depersisting the old Calib (FluxMag0/FluxMag0Err) objects.
def getLogger(loggername)