21 """Base class for BuildStars using src tables or sourceTable_visit tables.
31 import lsst.daf.persistence
as dafPersist
32 import lsst.pex.config
as pexConfig
33 import lsst.pipe.base
as pipeBase
34 import lsst.afw.table
as afwTable
35 import lsst.geom
as geom
36 from lsst.daf.base
import PropertyList
37 from lsst.daf.base.dateTime
import DateTime
38 from lsst.meas.algorithms.sourceSelector
import sourceSelectorRegistry
39 from lsst.utils.timer
import timeMethod
41 from .utilities
import computeApertureRadiusFromDataRef
42 from .fgcmLoadReferenceCatalog
import FgcmLoadReferenceCatalogTask
46 REFSTARS_FORMAT_VERSION = 1
48 __all__ = [
'FgcmBuildStarsConfigBase',
'FgcmBuildStarsRunner',
'FgcmBuildStarsBaseTask']
52 """Base config for FgcmBuildStars tasks"""
54 instFluxField = pexConfig.Field(
55 doc=(
"Faull name of the source instFlux field to use, including 'instFlux'. "
56 "The associated flag will be implicitly included in badFlags"),
58 default=
'slot_CalibFlux_instFlux',
60 minPerBand = pexConfig.Field(
61 doc=
"Minimum observations per band",
65 matchRadius = pexConfig.Field(
66 doc=
"Match radius (arcseconds)",
70 isolationRadius = pexConfig.Field(
71 doc=
"Isolation radius (arcseconds)",
75 densityCutNside = pexConfig.Field(
76 doc=
"Density cut healpix nside",
80 densityCutMaxPerPixel = pexConfig.Field(
81 doc=
"Density cut number of stars per pixel",
85 randomSeed = pexConfig.Field(
86 doc=
"Random seed for high density down-sampling.",
91 matchNside = pexConfig.Field(
92 doc=
"Healpix Nside for matching",
96 coarseNside = pexConfig.Field(
97 doc=
"Healpix coarse Nside for partitioning matches",
104 physicalFilterMap = pexConfig.DictField(
105 doc=
"Mapping from 'physicalFilter' to band.",
110 requiredBands = pexConfig.ListField(
111 doc=
"Bands required for each star",
115 primaryBands = pexConfig.ListField(
116 doc=(
"Bands for 'primary' star matches. "
117 "A star must be observed in one of these bands to be considered "
118 "as a calibration star."),
122 visitDataRefName = pexConfig.Field(
123 doc=
"dataRef name for the 'visit' field, usually 'visit'.",
127 ccdDataRefName = pexConfig.Field(
128 doc=
"dataRef name for the 'ccd' field, usually 'ccd' or 'detector'.",
132 doApplyWcsJacobian = pexConfig.Field(
133 doc=
"Apply the jacobian of the WCS to the star observations prior to fit?",
137 doModelErrorsWithBackground = pexConfig.Field(
138 doc=
"Model flux errors with background term?",
142 psfCandidateName = pexConfig.Field(
143 doc=
"Name of field with psf candidate flag for propagation",
145 default=
"calib_psf_candidate"
147 doSubtractLocalBackground = pexConfig.Field(
148 doc=(
"Subtract the local background before performing calibration? "
149 "This is only supported for circular aperture calibration fluxes."),
153 localBackgroundFluxField = pexConfig.Field(
154 doc=
"Full name of the local background instFlux field to use.",
156 default=
'base_LocalBackground_instFlux'
158 sourceSelector = sourceSelectorRegistry.makeField(
159 doc=
"How to select sources",
162 apertureInnerInstFluxField = pexConfig.Field(
163 doc=(
"Full name of instFlux field that contains inner aperture "
164 "flux for aperture correction proxy"),
166 default=
'base_CircularApertureFlux_12_0_instFlux'
168 apertureOuterInstFluxField = pexConfig.Field(
169 doc=(
"Full name of instFlux field that contains outer aperture "
170 "flux for aperture correction proxy"),
172 default=
'base_CircularApertureFlux_17_0_instFlux'
174 doReferenceMatches = pexConfig.Field(
175 doc=
"Match reference catalog as additional constraint on calibration",
179 fgcmLoadReferenceCatalog = pexConfig.ConfigurableField(
180 target=FgcmLoadReferenceCatalogTask,
181 doc=
"FGCM reference object loader",
183 nVisitsPerCheckpoint = pexConfig.Field(
184 doc=
"Number of visits read between checkpoints",
191 sourceSelector.setDefaults()
193 sourceSelector.doFlags =
True
194 sourceSelector.doUnresolved =
True
195 sourceSelector.doSignalToNoise =
True
196 sourceSelector.doIsolated =
True
198 sourceSelector.signalToNoise.minimum = 10.0
199 sourceSelector.signalToNoise.maximum = 1000.0
203 sourceSelector.unresolved.maximum = 0.5
207 """Subclass of TaskRunner for FgcmBuildStars tasks
209 fgcmBuildStarsTask.run() and fgcmBuildStarsTableTask.run() take a number of
210 arguments, one of which is the butler (for persistence and mapper data),
211 and a list of dataRefs extracted from the command line. Note that FGCM
212 runs on a large set of dataRefs, and not on single dataRef/tract/patch.
213 This class transforms the process arguments generated by the ArgumentParser
214 into the arguments expected by FgcmBuildStarsTask.run(). This runner does
215 not use any parallelization.
220 Return a list with one element: a tuple with the butler and
224 return [(parsedCmd.butler, parsedCmd.id.refList)]
230 args: `tuple` with (butler, dataRefList)
234 exitStatus: `list` with `lsst.pipe.base.Struct`
235 exitStatus (0: success; 1: failure)
237 butler, dataRefList = args
239 task = self.TaskClass(config=self.config, log=self.log)
243 task.runDataRef(butler, dataRefList)
246 task.runDataRef(butler, dataRefList)
247 except Exception
as e:
249 task.log.fatal(
"Failed: %s" % e)
250 if not isinstance(e, pipeBase.TaskError):
251 traceback.print_exc(file=sys.stderr)
253 task.writeMetadata(butler)
256 return [pipeBase.Struct(exitStatus=exitStatus)]
260 Run the task, with no multiprocessing
264 parsedCmd: `lsst.pipe.base.ArgumentParser` parsed command line
269 if self.precall(parsedCmd):
271 resultList = self(targetList[0])
278 Base task to build stars for FGCM global calibration
282 butler : `lsst.daf.persistence.Butler`
284 def __init__(self, initInputs=None, butler=None, **kwargs):
287 self.makeSubtask(
"sourceSelector")
289 self.sourceSelector.log.setLevel(self.sourceSelector.log.WARN)
292 def _getMetadataName(self):
298 Cross-match and make star list for FGCM Input
302 butler: `lsst.daf.persistence.Butler`
303 dataRefs: `list` of `lsst.daf.persistence.ButlerDataRef`
304 Source data references for the input visits.
308 RuntimeErrror: Raised if `config.doReferenceMatches` is set and
309 an fgcmLookUpTable is not available, or if computeFluxApertureRadius()
310 fails if the calibFlux is not a CircularAperture flux.
312 datasetType = dataRefs[0].butlerSubset.datasetType
313 self.log.info(
"Running with %d %s dataRefs", len(dataRefs), datasetType)
315 if self.config.doReferenceMatches:
316 self.makeSubtask(
"fgcmLoadReferenceCatalog", butler=butler)
318 if not butler.datasetExists(
'fgcmLookUpTable'):
319 raise RuntimeError(
"Must have fgcmLookUpTable if using config.doReferenceMatches")
322 calibFluxApertureRadius =
None
323 if self.config.doSubtractLocalBackground:
326 self.config.instFluxField)
327 except RuntimeError
as e:
328 raise RuntimeError(
"Could not determine aperture radius from %s. "
329 "Cannot use doSubtractLocalBackground." %
330 (self.config.instFluxField))
from e
332 camera = butler.get(
'camera')
340 visitCatDataRef = butler.dataRef(
'fgcmVisitCatalog')
341 filename = visitCatDataRef.get(
'fgcmVisitCatalog_filename')[0]
342 if os.path.exists(filename):
344 inVisitCat = visitCatDataRef.get()
345 if len(inVisitCat) != len(groupedDataRefs):
346 raise RuntimeError(
"Existing visitCatalog found, but has an inconsistent "
347 "number of visits. Cannot continue.")
352 visitCatDataRef=visitCatDataRef,
353 inVisitCat=inVisitCat)
356 visitCatDataRef.put(visitCat)
358 starObsDataRef = butler.dataRef(
'fgcmStarObservations')
359 filename = starObsDataRef.get(
'fgcmStarObservations_filename')[0]
360 if os.path.exists(filename):
361 inStarObsCat = starObsDataRef.get()
365 rad = calibFluxApertureRadius
366 sourceSchemaDataRef = butler.dataRef(
'src_schema')
367 sourceSchema = sourceSchemaDataRef.get(
'src_schema', immediate=
True).schema
372 calibFluxApertureRadius=rad,
373 starObsDataRef=starObsDataRef,
374 visitCatDataRef=visitCatDataRef,
375 inStarObsCat=inStarObsCat)
376 visitCatDataRef.put(visitCat)
377 starObsDataRef.put(fgcmStarObservationCat)
380 if self.config.doReferenceMatches:
381 lutDataRef = butler.dataRef(
'fgcmLookUpTable')
384 fgcmStarIdCat, fgcmStarIndicesCat, fgcmRefCat = self.
fgcmMatchStarsfgcmMatchStars(visitCat,
385 fgcmStarObservationCat,
386 lutDataRef=lutDataRef)
389 butler.put(fgcmStarIdCat,
'fgcmStarIds')
390 butler.put(fgcmStarIndicesCat,
'fgcmStarIndices')
391 if fgcmRefCat
is not None:
392 butler.put(fgcmRefCat,
'fgcmReferenceStars')
395 def _findAndGroupDataRefsGen2(self, butler, camera, dataRefs):
397 Find and group dataRefs (by visit); Gen2 only.
401 butler : `lsst.daf.persistence.Butler`
403 camera : `lsst.afw.cameraGeom.Camera`
404 Camera from the butler.
405 dataRefs : `list` of `lsst.daf.persistence.ButlerDataRef`
406 Data references for the input visits.
410 groupedDataRefs : `dict` [`int`, `list`]
411 Dictionary with sorted visit keys, and `list`s of
412 `lsst.daf.persistence.ButlerDataRef`
414 raise NotImplementedError(
"_findAndGroupDataRefsGen2 not implemented.")
420 calibFluxApertureRadius=None,
421 visitCatDataRef=None,
425 Compile all good star observations from visits in visitCat. Checkpoint files
426 will be stored if both visitCatDataRef and starObsDataRef are not None.
430 groupedDataRefs : `dict` of `list`s
431 Lists of `~lsst.daf.persistence.ButlerDataRef` or
432 `~lsst.daf.butler.DeferredDatasetHandle`, grouped by visit.
433 visitCat : `~afw.table.BaseCatalog`
434 Catalog with visit data for FGCM
435 sourceSchema : `~lsst.afw.table.Schema`
436 Schema for the input src catalogs.
437 camera : `~lsst.afw.cameraGeom.Camera`
438 calibFluxApertureRadius : `float`, optional
439 Aperture radius for calibration flux.
440 visitCatDataRef : `~lsst.daf.persistence.ButlerDataRef`, optional
441 Dataref to write visitCat for checkpoints
442 starObsDataRef : `~lsst.daf.persistence.ButlerDataRef`, optional
443 Dataref to write the star observation catalog for checkpoints.
444 inStarObsCat : `~afw.table.BaseCatalog`
445 Input observation catalog. If this is incomplete, observations
446 will be appended from when it was cut off.
450 fgcmStarObservations : `afw.table.BaseCatalog`
451 Full catalog of good observations.
455 RuntimeError: Raised if doSubtractLocalBackground is True and
456 calibFluxApertureRadius is not set.
458 raise NotImplementedError(
"fgcmMakeAllStarObservations not implemented.")
461 visitCatDataRef=None, inVisitCat=None):
463 Make a visit catalog with all the keys from each visit
467 camera: `lsst.afw.cameraGeom.Camera`
468 Camera from the butler
469 groupedDataRefs: `dict`
470 Dictionary with visit keys, and `list`s of
471 `lsst.daf.persistence.ButlerDataRef`
472 bkgDataRefDict: `dict`, optional
473 Dictionary of gen3 dataRefHandles for background info.
474 visitCatDataRef: `lsst.daf.persistence.ButlerDataRef`, optional
475 Dataref to write visitCat for checkpoints
476 inVisitCat: `afw.table.BaseCatalog`, optional
477 Input (possibly incomplete) visit catalog
481 visitCat: `afw.table.BaseCatalog`
484 self.log.info(
"Assembling visitCatalog from %d %ss" %
485 (len(groupedDataRefs), self.config.visitDataRefName))
489 if inVisitCat
is None:
492 visitCat = afwTable.BaseCatalog(schema)
493 visitCat.reserve(len(groupedDataRefs))
494 visitCat.resize(len(groupedDataRefs))
496 visitCat[
'visit'] = list(groupedDataRefs.keys())
498 visitCat[
'sources_read'] =
False
500 visitCat = inVisitCat
505 bkgDataRefDict=bkgDataRefDict,
506 visitCatDataRef=visitCatDataRef)
510 def _fillVisitCatalog(self, visitCat, groupedDataRefs, bkgDataRefDict=None,
511 visitCatDataRef=None):
513 Fill the visit catalog with visit metadata
517 visitCat : `afw.table.BaseCatalog`
518 Visit catalog. See _makeFgcmVisitSchema() for schema definition.
519 groupedDataRefs : `dict`
520 Dictionary with visit keys, and `list`s of
521 `lsst.daf.persistence.ButlerDataRef` or
522 `lsst.daf.butler.DeferredDatasetHandle`
523 visitCatDataRef : `lsst.daf.persistence.ButlerDataRef`, optional
524 Dataref to write ``visitCat`` for checkpoints. Gen2 only.
525 bkgDataRefDict : `dict`, optional
526 Dictionary of Gen3 `lsst.daf.butler.DeferredDatasetHandle`
529 bbox = geom.BoxI(geom.PointI(0, 0), geom.PointI(1, 1))
531 for i, visit
in enumerate(groupedDataRefs):
538 if visitCat[
'used'][i]:
541 if (i % self.config.nVisitsPerCheckpoint) == 0:
542 self.log.info(
"Retrieving metadata for %s %d (%d/%d)" %
543 (self.config.visitDataRefName, visit, i, len(groupedDataRefs)))
545 if visitCatDataRef
is not None:
546 visitCatDataRef.put(visitCat)
548 dataRef = groupedDataRefs[visit][0]
549 if isinstance(dataRef, dafPersist.ButlerDataRef):
552 exp = dataRef.get(datasetType=
'calexp_sub', bbox=bbox)
553 visitInfo = exp.getInfo().getVisitInfo()
554 label = dataRef.get(datasetType=
'calexp_filterLabel')
555 physicalFilter = label.physicalLabel
557 bbox = dataRef.get(datasetType=
'calexp_bbox')
558 psfSigma = psf.computeShape(bbox.getCenter()).getDeterminantRadius()
561 summary = dataRef.get()
563 summaryRow = summary.find(self.config.referenceCCD)
564 if summaryRow
is None:
566 summaryRow = summary[0]
568 summaryDetector = summaryRow[
'id']
569 visitInfo = summaryRow.getVisitInfo()
570 physicalFilter = summaryRow[
'physical_filter']
572 goodSigma, = np.where(summary[
'psfSigma'] > 0)
573 if goodSigma.size > 2:
574 psfSigma = np.median(summary[
'psfSigma'][goodSigma])
576 psfSigma = np.mean(summary[
'psfSigma'][goodSigma])
582 rec[
'physicalFilter'] = physicalFilter
586 radec = visitInfo.getBoresightRaDec()
587 rec[
'telra'] = radec.getRa().asDegrees()
588 rec[
'teldec'] = radec.getDec().asDegrees()
589 rec[
'telha'] = visitInfo.getBoresightHourAngle().asDegrees()
590 rec[
'telrot'] = visitInfo.getBoresightRotAngle().asDegrees()
591 rec[
'mjd'] = visitInfo.getDate().get(system=DateTime.MJD)
592 rec[
'exptime'] = visitInfo.getExposureTime()
595 rec[
'pmb'] = visitInfo.getWeather().getAirPressure() / 100
599 rec[
'scaling'][:] = 1.0
601 rec[
'deltaAper'] = 0.0
602 rec[
'psfSigma'] = psfSigma
604 if self.config.doModelErrorsWithBackground:
606 if isinstance(dataRef, dafPersist.ButlerDataRef):
608 det = dataRef.dataId[self.config.ccdDataRefName]
609 if dataRef.datasetExists(datasetType=
'calexpBackground'):
610 bgList = dataRef.get(datasetType=
'calexpBackground')
616 bkgRef = bkgDataRefDict[(visit, summaryDetector)]
617 bgList = bkgRef.get()
623 bgStats = (bg[0].getStatsImage().getImage().array
625 rec[
'skyBackground'] = sum(np.median(bg[np.isfinite(bg)])
for bg
in bgStats)
627 self.log.warning(
'Sky background not found for visit %d / ccd %d' %
629 rec[
'skyBackground'] = -1.0
631 rec[
'skyBackground'] = -1.0
635 def _makeSourceMapper(self, sourceSchema):
637 Make a schema mapper for fgcm sources
641 sourceSchema: `afwTable.Schema`
642 Default source schema from the butler
646 sourceMapper: `afwTable.schemaMapper`
647 Mapper to the FGCM source schema
651 sourceMapper = afwTable.SchemaMapper(sourceSchema)
654 sourceMapper.addMapping(sourceSchema[
'coord_ra'].asKey(),
'ra')
655 sourceMapper.addMapping(sourceSchema[
'coord_dec'].asKey(),
'dec')
656 sourceMapper.addMapping(sourceSchema[
'slot_Centroid_x'].asKey(),
'x')
657 sourceMapper.addMapping(sourceSchema[
'slot_Centroid_y'].asKey(),
'y')
663 sourceMapper.addMapping(sourceSchema[self.config.psfCandidateName].asKey(),
666 sourceMapper.editOutputSchema().addField(
667 "psf_candidate", type=
'Flag',
668 doc=(
"Flag set if the source was a candidate for PSF determination, "
669 "as determined by the star selector."))
672 sourceMapper.editOutputSchema().addField(
673 "visit", type=np.int32, doc=
"Visit number")
674 sourceMapper.editOutputSchema().addField(
675 "ccd", type=np.int32, doc=
"CCD number")
676 sourceMapper.editOutputSchema().addField(
677 "instMag", type=np.float32, doc=
"Instrumental magnitude")
678 sourceMapper.editOutputSchema().addField(
679 "instMagErr", type=np.float32, doc=
"Instrumental magnitude error")
680 sourceMapper.editOutputSchema().addField(
681 "jacobian", type=np.float32, doc=
"Relative pixel scale from wcs jacobian")
682 sourceMapper.editOutputSchema().addField(
683 "deltaMagBkg", type=np.float32, doc=
"Change in magnitude due to local background offset")
689 Use FGCM code to match observations into unique stars.
693 visitCat: `afw.table.BaseCatalog`
694 Catalog with visit data for fgcm
695 obsCat: `afw.table.BaseCatalog`
696 Full catalog of star observations for fgcm
697 lutDataRef: `lsst.daf.persistence.ButlerDataRef` or
698 `lsst.daf.butler.DeferredDatasetHandle`, optional
699 Data reference to fgcm look-up table (used if matching reference stars).
703 fgcmStarIdCat: `afw.table.BaseCatalog`
704 Catalog of unique star identifiers and index keys
705 fgcmStarIndicesCat: `afwTable.BaseCatalog`
706 Catalog of unique star indices
707 fgcmRefCat: `afw.table.BaseCatalog`
708 Catalog of matched reference stars.
709 Will be None if `config.doReferenceMatches` is False.
713 visitFilterNames = np.zeros(len(visitCat), dtype=
'a30')
714 for i
in range(len(visitCat)):
715 visitFilterNames[i] = visitCat[i][
'physicalFilter']
718 visitIndex = np.searchsorted(visitCat[
'visit'],
721 obsFilterNames = visitFilterNames[visitIndex]
723 if self.config.doReferenceMatches:
725 lutCat = lutDataRef.get()
727 stdFilterDict = {filterName: stdFilter
for (filterName, stdFilter)
in
728 zip(lutCat[0][
'physicalFilters'].split(
','),
729 lutCat[0][
'stdPhysicalFilters'].split(
','))}
730 stdLambdaDict = {stdFilter: stdLambda
for (stdFilter, stdLambda)
in
731 zip(lutCat[0][
'stdPhysicalFilters'].split(
','),
732 lutCat[0][
'lambdaStdFilter'])}
739 self.log.info(
"Using the following reference filters: %s" %
740 (
', '.join(referenceFilterNames)))
744 referenceFilterNames = []
747 starConfig = {
'logger': self.log,
748 'filterToBand': self.config.physicalFilterMap,
749 'requiredBands': self.config.requiredBands,
750 'minPerBand': self.config.minPerBand,
751 'matchRadius': self.config.matchRadius,
752 'isolationRadius': self.config.isolationRadius,
753 'matchNSide': self.config.matchNside,
754 'coarseNSide': self.config.coarseNside,
755 'densNSide': self.config.densityCutNside,
756 'densMaxPerPixel': self.config.densityCutMaxPerPixel,
757 'randomSeed': self.config.randomSeed,
758 'primaryBands': self.config.primaryBands,
759 'referenceFilterNames': referenceFilterNames}
762 fgcmMakeStars = fgcm.FgcmMakeStars(starConfig)
770 conv = obsCat[0][
'ra'].asDegrees() / float(obsCat[0][
'ra'])
771 fgcmMakeStars.makePrimaryStars(obsCat[
'ra'] * conv,
772 obsCat[
'dec'] * conv,
773 filterNameArray=obsFilterNames,
777 fgcmMakeStars.makeMatchedStars(obsCat[
'ra'] * conv,
778 obsCat[
'dec'] * conv,
781 if self.config.doReferenceMatches:
782 fgcmMakeStars.makeReferenceMatches(self.fgcmLoadReferenceCatalog)
789 fgcmStarIdCat = afwTable.BaseCatalog(objSchema)
790 fgcmStarIdCat.reserve(fgcmMakeStars.objIndexCat.size)
791 for i
in range(fgcmMakeStars.objIndexCat.size):
792 fgcmStarIdCat.addNew()
795 fgcmStarIdCat[
'fgcm_id'][:] = fgcmMakeStars.objIndexCat[
'fgcm_id']
796 fgcmStarIdCat[
'ra'][:] = fgcmMakeStars.objIndexCat[
'ra']
797 fgcmStarIdCat[
'dec'][:] = fgcmMakeStars.objIndexCat[
'dec']
798 fgcmStarIdCat[
'obsArrIndex'][:] = fgcmMakeStars.objIndexCat[
'obsarrindex']
799 fgcmStarIdCat[
'nObs'][:] = fgcmMakeStars.objIndexCat[
'nobs']
803 fgcmStarIndicesCat = afwTable.BaseCatalog(obsSchema)
804 fgcmStarIndicesCat.reserve(fgcmMakeStars.obsIndexCat.size)
805 for i
in range(fgcmMakeStars.obsIndexCat.size):
806 fgcmStarIndicesCat.addNew()
808 fgcmStarIndicesCat[
'obsIndex'][:] = fgcmMakeStars.obsIndexCat[
'obsindex']
810 if self.config.doReferenceMatches:
813 fgcmRefCat = afwTable.BaseCatalog(refSchema)
814 fgcmRefCat.reserve(fgcmMakeStars.referenceCat.size)
816 for i
in range(fgcmMakeStars.referenceCat.size):
819 fgcmRefCat[
'fgcm_id'][:] = fgcmMakeStars.referenceCat[
'fgcm_id']
820 fgcmRefCat[
'refMag'][:, :] = fgcmMakeStars.referenceCat[
'refMag']
821 fgcmRefCat[
'refMagErr'][:, :] = fgcmMakeStars.referenceCat[
'refMagErr']
824 md.set(
"REFSTARS_FORMAT_VERSION", REFSTARS_FORMAT_VERSION)
825 md.set(
"FILTERNAMES", referenceFilterNames)
826 fgcmRefCat.setMetadata(md)
831 return fgcmStarIdCat, fgcmStarIndicesCat, fgcmRefCat
833 def _makeFgcmVisitSchema(self, nCcd):
835 Make a schema for an fgcmVisitCatalog
840 Number of CCDs in the camera
844 schema: `afwTable.Schema`
847 schema = afwTable.Schema()
848 schema.addField(
'visit', type=np.int32, doc=
"Visit number")
849 schema.addField(
'physicalFilter', type=str, size=30, doc=
"Physical filter")
850 schema.addField(
'telra', type=np.float64, doc=
"Pointing RA (deg)")
851 schema.addField(
'teldec', type=np.float64, doc=
"Pointing Dec (deg)")
852 schema.addField(
'telha', type=np.float64, doc=
"Pointing Hour Angle (deg)")
853 schema.addField(
'telrot', type=np.float64, doc=
"Camera rotation (deg)")
854 schema.addField(
'mjd', type=np.float64, doc=
"MJD of visit")
855 schema.addField(
'exptime', type=np.float32, doc=
"Exposure time")
856 schema.addField(
'pmb', type=np.float32, doc=
"Pressure (millibar)")
857 schema.addField(
'psfSigma', type=np.float32, doc=
"PSF sigma (reference CCD)")
858 schema.addField(
'deltaAper', type=np.float32, doc=
"Delta-aperture")
859 schema.addField(
'skyBackground', type=np.float32, doc=
"Sky background (ADU) (reference CCD)")
861 schema.addField(
'deepFlag', type=np.int32, doc=
"Deep observation")
862 schema.addField(
'scaling', type=
'ArrayD', doc=
"Scaling applied due to flat adjustment",
864 schema.addField(
'used', type=np.int32, doc=
"This visit has been ingested.")
865 schema.addField(
'sources_read', type=
'Flag', doc=
"This visit had sources read.")
869 def _makeFgcmObjSchema(self):
871 Make a schema for the objIndexCat from fgcmMakeStars
875 schema: `afwTable.Schema`
878 objSchema = afwTable.Schema()
879 objSchema.addField(
'fgcm_id', type=np.int32, doc=
'FGCM Unique ID')
881 objSchema.addField(
'ra', type=np.float64, doc=
'Mean object RA (deg)')
882 objSchema.addField(
'dec', type=np.float64, doc=
'Mean object Dec (deg)')
883 objSchema.addField(
'obsArrIndex', type=np.int32,
884 doc=
'Index in obsIndexTable for first observation')
885 objSchema.addField(
'nObs', type=np.int32, doc=
'Total number of observations')
889 def _makeFgcmObsSchema(self):
891 Make a schema for the obsIndexCat from fgcmMakeStars
895 schema: `afwTable.Schema`
898 obsSchema = afwTable.Schema()
899 obsSchema.addField(
'obsIndex', type=np.int32, doc=
'Index in observation table')
903 def _makeFgcmRefSchema(self, nReferenceBands):
905 Make a schema for the referenceCat from fgcmMakeStars
909 nReferenceBands: `int`
910 Number of reference bands
914 schema: `afwTable.Schema`
917 refSchema = afwTable.Schema()
918 refSchema.addField(
'fgcm_id', type=np.int32, doc=
'FGCM Unique ID')
919 refSchema.addField(
'refMag', type=
'ArrayF', doc=
'Reference magnitude array (AB)',
920 size=nReferenceBands)
921 refSchema.addField(
'refMagErr', type=
'ArrayF', doc=
'Reference magnitude error array',
922 size=nReferenceBands)
926 def _getReferenceFilterNames(self, visitCat, stdFilterDict, stdLambdaDict):
928 Get the reference filter names, in wavelength order, from the visitCat and
929 information from the look-up-table.
933 visitCat: `afw.table.BaseCatalog`
934 Catalog with visit data for FGCM
935 stdFilterDict: `dict`
936 Mapping of filterName to stdFilterName from LUT
937 stdLambdaDict: `dict`
938 Mapping of stdFilterName to stdLambda from LUT
942 referenceFilterNames: `list`
943 Wavelength-ordered list of reference filter names
947 filterNames = np.unique(visitCat.asAstropy()[
'physicalFilter'])
950 stdFilterNames = {stdFilterDict[filterName]
for filterName
in filterNames}
953 referenceFilterNames = sorted(stdFilterNames, key=stdLambdaDict.get)
955 return referenceFilterNames
def fgcmMatchStars(self, visitCat, obsCat, lutDataRef=None)
def _makeFgcmVisitSchema(self, nCcd)
def _getReferenceFilterNames(self, visitCat, stdFilterDict, stdLambdaDict)
def runDataRef(self, butler, dataRefs)
def _makeFgcmObjSchema(self)
def _fillVisitCatalog(self, visitCat, groupedDataRefs, bkgDataRefDict=None, visitCatDataRef=None)
def fgcmMakeAllStarObservations(self, groupedDataRefs, visitCat, sourceSchema, camera, calibFluxApertureRadius=None, visitCatDataRef=None, starObsDataRef=None, inStarObsCat=None)
def __init__(self, initInputs=None, butler=None, **kwargs)
def _makeFgcmObsSchema(self)
def fgcmMakeVisitCatalog(self, camera, groupedDataRefs, bkgDataRefDict=None, visitCatDataRef=None, inVisitCat=None)
def _findAndGroupDataRefsGen2(self, butler, camera, dataRefs)
def _makeFgcmRefSchema(self, nReferenceBands)
def getTargetList(parsedCmd)
def computeApertureRadiusFromDataRef(dataRef, fluxField)