imageDifference.py

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# This file is part of pipe_tasks.
#
# Developed for the LSST Data Management System.
# This product includes software developed by the LSST Project
# (https://www.lsst.org).
# See the COPYRIGHT file at the top-level directory of this distribution
# for details of code ownership.
#
# This program is free software: you can redistribute it and/or modify
# it under the terms of the GNU General Public License as published by
# the Free Software Foundation, either version 3 of the License, or
# (at your option) any later version.
#
# This program is distributed in the hope that it will be useful,
# but WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the
# GNU General Public License for more details.
#
# You should have received a copy of the GNU General Public License
# along with this program.  If not, see <https://www.gnu.org/licenses/>.
 
__all__ = ["ImageDifferenceConfig", "ImageDifferenceTask"]
 
import math
import random
import numpy
 
import lsst.utils
import lsst.pex.config as pexConfig
import lsst.pipe.base as pipeBase
import lsst.daf.base as dafBase
import lsst.geom as geom
import lsst.afw.math as afwMath
import lsst.afw.table as afwTable
import lsst.meas.extensions.trailedSources  # noqa: F401
from lsst.meas.algorithms import (SourceDetectionTask, SingleGaussianPsf, ObjectSizeStarSelectorTask,
                                  LoadReferenceObjectsConfig, SkyObjectsTask,
                                  ScaleVarianceTask)
from lsst.meas.astrom import AstrometryConfig, AstrometryTask
from lsst.meas.base import ForcedMeasurementTask, ApplyApCorrTask
from lsst.pipe.tasks.registerImage import RegisterTask
from lsst.ip.diffim import (DipoleAnalysis, SourceFlagChecker, KernelCandidateF, makeKernelBasisList,
                            KernelCandidateQa, DiaCatalogSourceSelectorTask, DiaCatalogSourceSelectorConfig,
                            GetCoaddAsTemplateTask, DipoleFitTask,
                            DecorrelateALKernelSpatialTask, subtractAlgorithmRegistry)
import lsst.ip.diffim.diffimTools as diffimTools
import lsst.ip.diffim.utils as diUtils
import lsst.afw.display as afwDisplay
from lsst.skymap import BaseSkyMap
from lsst.obs.base import ExposureIdInfo
from lsst.utils.timer import timeMethod
 
from deprecated.sphinx import deprecated
 
FwhmPerSigma = 2*math.sqrt(2*math.log(2))
IqrToSigma = 0.741
 
 
class ImageDifferenceTaskConnections(pipeBase.PipelineTaskConnections,
                                     dimensions=("instrument", "visit", "detector", "skymap"),
                                     defaultTemplates={"coaddName": "deep",
                                                       "skyMapName": "deep",
                                                       "warpTypeSuffix": "",
                                                       "fakesType": ""}):
 
    exposure = pipeBase.connectionTypes.Input(
        doc="Input science exposure to subtract from.",
        dimensions=("instrument", "visit", "detector"),
        storageClass="ExposureF",
        name="{fakesType}calexp"
    )
 
    # TODO DM-22953
    # kernelSources = pipeBase.connectionTypes.Input(
    #     doc="Source catalog produced in calibrate task for kernel candidate sources",
    #     name="src",
    #     storageClass="SourceCatalog",
    #     dimensions=("instrument", "visit", "detector"),
    # )
 
    skyMap = pipeBase.connectionTypes.Input(
        doc="Input definition of geometry/bbox and projection/wcs for template exposures",
        name=BaseSkyMap.SKYMAP_DATASET_TYPE_NAME,
        dimensions=("skymap", ),
        storageClass="SkyMap",
    )
    coaddExposures = pipeBase.connectionTypes.Input(
        doc="Input template to match and subtract from the exposure",
        dimensions=("tract", "patch", "skymap", "band"),
        storageClass="ExposureF",
        name="{fakesType}{coaddName}Coadd{warpTypeSuffix}",
        multiple=True,
        deferLoad=True
    )
    dcrCoadds = pipeBase.connectionTypes.Input(
        doc="Input DCR template to match and subtract from the exposure",
        name="{fakesType}dcrCoadd{warpTypeSuffix}",
        storageClass="ExposureF",
        dimensions=("tract", "patch", "skymap", "band", "subfilter"),
        multiple=True,
        deferLoad=True
    )
    finalizedPsfApCorrCatalog = pipeBase.connectionTypes.Input(
        doc=("Per-visit finalized psf models and aperture correction maps. "
             "These catalogs use the detector id for the catalog id, "
             "sorted on id for fast lookup."),
        name="finalized_psf_ap_corr_catalog",
        storageClass="ExposureCatalog",
        dimensions=("instrument", "visit"),
    )
    outputSchema = pipeBase.connectionTypes.InitOutput(
        doc="Schema (as an example catalog) for output DIASource catalog.",
        storageClass="SourceCatalog",
        name="{fakesType}{coaddName}Diff_diaSrc_schema",
    )
    subtractedExposure = pipeBase.connectionTypes.Output(
        doc="Output AL difference or Zogy proper difference image",
        dimensions=("instrument", "visit", "detector"),
        storageClass="ExposureF",
        name="{fakesType}{coaddName}Diff_differenceExp",
    )
    scoreExposure = pipeBase.connectionTypes.Output(
        doc="Output AL likelihood or Zogy score image",
        dimensions=("instrument", "visit", "detector"),
        storageClass="ExposureF",
        name="{fakesType}{coaddName}Diff_scoreExp",
    )
    warpedExposure = pipeBase.connectionTypes.Output(
        doc="Warped template used to create `subtractedExposure`.",
        dimensions=("instrument", "visit", "detector"),
        storageClass="ExposureF",
        name="{fakesType}{coaddName}Diff_warpedExp",
    )
    matchedExposure = pipeBase.connectionTypes.Output(
        doc="Warped template used to create `subtractedExposure`.",
        dimensions=("instrument", "visit", "detector"),
        storageClass="ExposureF",
        name="{fakesType}{coaddName}Diff_matchedExp",
    )
    diaSources = pipeBase.connectionTypes.Output(
        doc="Output detected diaSources on the difference image",
        dimensions=("instrument", "visit", "detector"),
        storageClass="SourceCatalog",
        name="{fakesType}{coaddName}Diff_diaSrc",
    )
 
    def __init__(self, *, config=None):
        super().__init__(config=config)
        if config.coaddName == 'dcr':
            self.inputs.remove("coaddExposures")
        else:
            self.inputs.remove("dcrCoadds")
        if not config.doWriteSubtractedExp:
            self.outputs.remove("subtractedExposure")
        if not config.doWriteScoreExp:
            self.outputs.remove("scoreExposure")
        if not config.doWriteWarpedExp:
            self.outputs.remove("warpedExposure")
        if not config.doWriteMatchedExp:
            self.outputs.remove("matchedExposure")
        if not config.doWriteSources:
            self.outputs.remove("diaSources")
        if not config.doApplyFinalizedPsf:
            self.inputs.remove("finalizedPsfApCorrCatalog")
 
    # TODO DM-22953: Add support for refObjLoader (kernelSourcesFromRef)
    # Make kernelSources optional
 
 
class ImageDifferenceConfig(pipeBase.PipelineTaskConfig,
                            pipelineConnections=ImageDifferenceTaskConnections):
    """Config for ImageDifferenceTask.
    """
 
    doAddCalexpBackground = pexConfig.Field(dtype=bool, default=False,
                                            doc="Add background to calexp before processing it.  "
                                                "Useful as ipDiffim does background matching.")
    doUseRegister = pexConfig.Field(dtype=bool, default=False,
                                    doc="Re-compute astrometry on the template. "
                                    "Use image-to-image registration to align template with "
                                    "science image (AL only).")
    doDebugRegister = pexConfig.Field(dtype=bool, default=False,
                                      doc="Writing debugging data for doUseRegister")
    doSelectSources = pexConfig.Field(dtype=bool, default=False,
                                      doc="Select stars to use for kernel fitting (AL only)")
    doSelectDcrCatalog = pexConfig.Field(dtype=bool, default=False,
                                         doc="Select stars of extreme color as part "
                                         "of the control sample (AL only)")
    doSelectVariableCatalog = pexConfig.Field(dtype=bool, default=False,
                                              doc="Select stars that are variable to be part "
                                                  "of the control sample (AL only)")
    doSubtract = pexConfig.Field(dtype=bool, default=True, doc="Compute subtracted exposure?")
    doPreConvolve = pexConfig.Field(dtype=bool, default=False,
                                    doc="Not in use. Superseded by useScoreImageDetection.",
                                    deprecated="This option superseded by useScoreImageDetection."
                                    " Will be removed after v22.")
    useScoreImageDetection = pexConfig.Field(
        dtype=bool, default=False, doc="Calculate the pre-convolved AL likelihood or "
        "the Zogy score image. Use it for source detection (if doDetection=True).")
    doWriteScoreExp = pexConfig.Field(
        dtype=bool, default=False, doc="Write AL likelihood or Zogy score exposure?")
    doScaleTemplateVariance = pexConfig.Field(dtype=bool, default=False,
                                              doc="Scale variance of the template before PSF matching")
    doScaleDiffimVariance = pexConfig.Field(dtype=bool, default=True,
                                            doc="Scale variance of the diffim before PSF matching. "
                                                "You may do either this or template variance scaling, "
                                                "or neither. (Doing both is a waste of CPU.)")
    useGaussianForPreConvolution = pexConfig.Field(
        dtype=bool, default=False, doc="Use a simple gaussian PSF model for pre-convolution "
        "(oherwise use exposure PSF)? (AL and if useScoreImageDetection=True only)")
    doDetection = pexConfig.Field(dtype=bool, default=True, doc="Detect sources?")
    doDecorrelation = pexConfig.Field(dtype=bool, default=True,
                                      doc="Perform diffim decorrelation to undo pixel correlation due to A&L "
                                      "kernel convolution (AL only)? If True, also update the diffim PSF.")
    doMerge = pexConfig.Field(dtype=bool, default=True,
                              doc="Merge positive and negative diaSources with grow radius "
                                  "set by growFootprint")
    doMatchSources = pexConfig.Field(dtype=bool, default=False,
                                     doc="Match diaSources with input calexp sources and ref catalog sources")
    doMeasurement = pexConfig.Field(dtype=bool, default=True, doc="Measure diaSources?")
    doDipoleFitting = pexConfig.Field(dtype=bool, default=True, doc="Measure dipoles using new algorithm?")
    doForcedMeasurement = pexConfig.Field(
        dtype=bool,
        default=True,
        doc="Force photometer diaSource locations on PVI?")
    doWriteSubtractedExp = pexConfig.Field(
        dtype=bool, default=True, doc="Write difference exposure (AL and Zogy) ?")
    doWriteWarpedExp = pexConfig.Field(
        dtype=bool, default=False, doc="Write WCS, warped template coadd exposure?")
    doWriteMatchedExp = pexConfig.Field(dtype=bool, default=False,
                                        doc="Write warped and PSF-matched template coadd exposure?")
    doWriteSources = pexConfig.Field(dtype=bool, default=True, doc="Write sources?")
    doAddMetrics = pexConfig.Field(dtype=bool, default=False,
                                   doc="Add columns to the source table to hold analysis metrics?")
    doApplyFinalizedPsf = pexConfig.Field(
        doc="Whether to apply finalized psf models and aperture correction map.",
        dtype=bool,
        default=False,
    )
 
    coaddName = pexConfig.Field(
        doc="coadd name: typically one of deep, goodSeeing, or dcr",
        dtype=str,
        default="deep",
    )
    convolveTemplate = pexConfig.Field(
        doc="Which image gets convolved (default = template)",
        dtype=bool,
        default=True
    )
    refObjLoader = pexConfig.ConfigField(
        dtype=LoadReferenceObjectsConfig,
        doc="reference object loader",
    )
    astrometer = pexConfig.ConfigurableField(
        target=AstrometryTask,
        doc="astrometry task; used to match sources to reference objects, but not to fit a WCS",
    )
    sourceSelector = pexConfig.ConfigurableField(
        target=ObjectSizeStarSelectorTask,
        doc="Source selection algorithm",
    )
    subtract = subtractAlgorithmRegistry.makeField("Subtraction Algorithm", default="al")
    decorrelate = pexConfig.ConfigurableField(
        target=DecorrelateALKernelSpatialTask,
        doc="Decorrelate effects of A&L kernel convolution on image difference, only if doSubtract is True. "
        "If this option is enabled, then detection.thresholdValue should be set to 5.0 (rather than the "
        "default of 5.5).",
    )
    # Old style ImageMapper grid. ZogyTask has its own grid option
    doSpatiallyVarying = pexConfig.Field(
        dtype=bool,
        default=False,
        doc="Perform A&L decorrelation on a grid across the "
        "image in order to allow for spatial variations. Zogy does not use this option."
    )
    detection = pexConfig.ConfigurableField(
        target=SourceDetectionTask,
        doc="Low-threshold detection for final measurement",
    )
    measurement = pexConfig.ConfigurableField(
        target=DipoleFitTask,
        doc="Enable updated dipole fitting method",
    )
    doApCorr = lsst.pex.config.Field(
        dtype=bool,
        default=True,
        doc="Run subtask to apply aperture corrections"
    )
    applyApCorr = lsst.pex.config.ConfigurableField(
        target=ApplyApCorrTask,
        doc="Subtask to apply aperture corrections"
    )
    forcedMeasurement = pexConfig.ConfigurableField(
        target=ForcedMeasurementTask,
        doc="Subtask to force photometer PVI at diaSource location.",
    )
    getTemplate = pexConfig.ConfigurableField(
        target=GetCoaddAsTemplateTask,
        doc="Subtask to retrieve template exposure and sources",
    )
    scaleVariance = pexConfig.ConfigurableField(
        target=ScaleVarianceTask,
        doc="Subtask to rescale the variance of the template "
            "to the statistically expected level"
    )
    controlStepSize = pexConfig.Field(
        doc="What step size (every Nth one) to select a control sample from the kernelSources",
        dtype=int,
        default=5
    )
    controlRandomSeed = pexConfig.Field(
        doc="Random seed for shuffing the control sample",
        dtype=int,
        default=10
    )
    register = pexConfig.ConfigurableField(
        target=RegisterTask,
        doc="Task to enable image-to-image image registration (warping)",
    )
    kernelSourcesFromRef = pexConfig.Field(
        doc="Select sources to measure kernel from reference catalog if True, template if false",
        dtype=bool,
        default=False
    )
    templateSipOrder = pexConfig.Field(
        dtype=int, default=2,
        doc="Sip Order for fitting the Template Wcs (default is too high, overfitting)"
    )
    growFootprint = pexConfig.Field(
        dtype=int, default=2,
        doc="Grow positive and negative footprints by this amount before merging"
    )
    diaSourceMatchRadius = pexConfig.Field(
        dtype=float, default=0.5,
        doc="Match radius (in arcseconds) for DiaSource to Source association"
    )
    requiredTemplateFraction = pexConfig.Field(
        dtype=float, default=0.1,
        doc="Do not attempt to run task if template covers less than this fraction of pixels."
        "Setting to 0 will always attempt image subtraction"
    )
    doSkySources = pexConfig.Field(
        dtype=bool,
        default=False,
        doc="Generate sky sources?",
    )
    skySources = pexConfig.ConfigurableField(
        target=SkyObjectsTask,
        doc="Generate sky sources",
    )
 
    def setDefaults(self):
        # defaults are OK for catalog and diacatalog
 
        self.subtract['al'].kernel.name = "AL"
        self.subtract['al'].kernel.active.fitForBackground = True
        self.subtract['al'].kernel.active.spatialKernelOrder = 1
        self.subtract['al'].kernel.active.spatialBgOrder = 2
 
        # DiaSource Detection
        self.detection.thresholdPolarity = "both"
        self.detection.thresholdValue = 5.0
        self.detection.reEstimateBackground = False
        self.detection.thresholdType = "pixel_stdev"
 
        # Add filtered flux measurement, the correct measurement for pre-convolved images.
        # Enable all measurements, regardless of doPreConvolve, as it makes data harvesting easier.
        # To change that you must modify algorithms.names in the task's applyOverrides method,
        # after the user has set doPreConvolve.
        self.measurement.algorithms.names.add('base_PeakLikelihoodFlux')
        self.measurement.plugins.names |= ['ext_trailedSources_Naive',
                                           'base_LocalPhotoCalib',
                                           'base_LocalWcs']
 
        self.forcedMeasurement.plugins = ["base_TransformedCentroid", "base_PsfFlux"]
        self.forcedMeasurement.copyColumns = {
            "id": "objectId", "parent": "parentObjectId", "coord_ra": "coord_ra", "coord_dec": "coord_dec"}
        self.forcedMeasurement.slots.centroid = "base_TransformedCentroid"
        self.forcedMeasurement.slots.shape = None
 
        # For shuffling the control sample
        random.seed(self.controlRandomSeed)
 
    def validate(self):
        pexConfig.Config.validate(self)
        if not self.doSubtract and not self.doDetection:
            raise ValueError("Either doSubtract or doDetection must be enabled.")
        if self.doMeasurement and not self.doDetection:
            raise ValueError("Cannot run source measurement without source detection.")
        if self.doMerge and not self.doDetection:
            raise ValueError("Cannot run source merging without source detection.")
        if self.doSkySources and not self.doDetection:
            raise ValueError("Cannot run sky source creation without source detection.")
        if self.doUseRegister and not self.doSelectSources:
            raise ValueError("doUseRegister=True and doSelectSources=False. "
                             "Cannot run RegisterTask without selecting sources.")
        if self.doScaleDiffimVariance and self.doScaleTemplateVariance:
            raise ValueError("Scaling the diffim variance and scaling the template variance "
                             "are both set. Please choose one or the other.")
        # We cannot allow inconsistencies that would lead to None or not available output products
        if self.subtract.name == 'zogy':
            if self.doWriteMatchedExp:
                raise ValueError("doWriteMatchedExp=True Matched exposure is not "
                                 "calculated in zogy subtraction.")
            if self.doAddMetrics:
                raise ValueError("doAddMetrics=True Kernel metrics does not exist in zogy subtraction.")
            if self.doDecorrelation:
                raise ValueError(
                    "doDecorrelation=True The decorrelation afterburner does not exist in zogy subtraction.")
            if self.doSelectSources:
                raise ValueError(
                    "doSelectSources=True Selecting sources for PSF matching is not a zogy option.")
            if self.useGaussianForPreConvolution:
                raise ValueError(
                    "useGaussianForPreConvolution=True This is an AL subtraction only option.")
        else:
            # AL only consistency checks
            if self.useScoreImageDetection and not self.convolveTemplate:
                raise ValueError(
                    "convolveTemplate=False and useScoreImageDetection=True "
                    "Pre-convolution and matching of the science image is not a supported operation.")
            if self.doWriteSubtractedExp and self.useScoreImageDetection:
                raise ValueError(
                    "doWriteSubtractedExp=True and useScoreImageDetection=True "
                    "Regular difference image is not calculated. "
                    "AL subtraction calculates either the regular difference image or the score image.")
            if self.doWriteScoreExp and not self.useScoreImageDetection:
                raise ValueError(
                    "doWriteScoreExp=True and useScoreImageDetection=False "
                    "Score image is not calculated. "
                    "AL subtraction calculates either the regular difference image or the score image.")
            if self.doAddMetrics and not self.doSubtract:
                raise ValueError("Subtraction must be enabled for kernel metrics calculation.")
            if self.useGaussianForPreConvolution and not self.useScoreImageDetection:
                raise ValueError(
                    "useGaussianForPreConvolution=True and useScoreImageDetection=False "
                    "Gaussian PSF approximation exists only for AL subtraction w/ pre-convolution.")
 
 
@deprecated(reason="This Task has been replaced with lsst.ip.diffim.subtractImages"
            " and lsst.ip.diffim.detectAndMeasure. Will be removed after v25.",
            version="v24.0", category=FutureWarning)
class ImageDifferenceTask(pipeBase.PipelineTask):
    """Subtract an image from a template and measure the result.
 
    Parameters
    ----------
    butler : `lsst.daf.butler.Butler` or `None`, optional
        Butler object to use in constructing reference object loaders.
    **kwargs
        Additional keyword arguments.
    """
    ConfigClass = ImageDifferenceConfig
    _DefaultName = "imageDifference"
 
    def __init__(self, butler=None, **kwargs):
        super().__init__(**kwargs)
        self.makeSubtask("getTemplate")
 
        self.makeSubtask("subtract")
 
        if self.config.subtract.name == 'al' and self.config.doDecorrelation:
            self.makeSubtask("decorrelate")
 
        if self.config.doScaleTemplateVariance or self.config.doScaleDiffimVariance:
            self.makeSubtask("scaleVariance")
 
        if self.config.doUseRegister:
            self.makeSubtask("register")
        self.schema = afwTable.SourceTable.makeMinimalSchema()
 
        if self.config.doSelectSources:
            self.makeSubtask("sourceSelector")
            if self.config.kernelSourcesFromRef:
                self.makeSubtask('refObjLoader', butler=butler)
                self.makeSubtask("astrometer", refObjLoader=self.refObjLoader)
 
        self.algMetadata = dafBase.PropertyList()
        if self.config.doDetection:
            self.makeSubtask("detection", schema=self.schema)
        if self.config.doMeasurement:
            self.makeSubtask("measurement", schema=self.schema,
                             algMetadata=self.algMetadata)
        if self.config.doApCorr:
            self.makeSubtask("applyApCorr", schema=self.measurement.schema)
        if self.config.doForcedMeasurement:
            self.schema.addField(
                "ip_diffim_forced_PsfFlux_instFlux", "D",
                "Forced PSF flux measured on the direct image.",
                units="count")
            self.schema.addField(
                "ip_diffim_forced_PsfFlux_instFluxErr", "D",
                "Forced PSF flux error measured on the direct image.",
                units="count")
            self.schema.addField(
                "ip_diffim_forced_PsfFlux_area", "F",
                "Forced PSF flux effective area of PSF.",
                units="pixel")
            self.schema.addField(
                "ip_diffim_forced_PsfFlux_flag", "Flag",
                "Forced PSF flux general failure flag.")
            self.schema.addField(
                "ip_diffim_forced_PsfFlux_flag_noGoodPixels", "Flag",
                "Forced PSF flux not enough non-rejected pixels in data to attempt the fit.")
            self.schema.addField(
                "ip_diffim_forced_PsfFlux_flag_edge", "Flag",
                "Forced PSF flux object was too close to the edge of the image to use the full PSF model.")
            self.makeSubtask("forcedMeasurement", refSchema=self.schema)
        if self.config.doMatchSources:
            self.schema.addField("refMatchId", "L", "unique id of reference catalog match")
            self.schema.addField("srcMatchId", "L", "unique id of source match")
        if self.config.doSkySources:
            self.makeSubtask("skySources")
            self.skySourceKey = self.schema.addField("sky_source", type="Flag", doc="Sky objects.")
 
        # initialize InitOutputs
        self.outputSchema = afwTable.SourceCatalog(self.schema)
        self.outputSchema.getTable().setMetadata(self.algMetadata)
 
    @staticmethod
    def makeIdFactory(expId, expBits):
        """Create IdFactory instance for unique 64 bit diaSource id-s.
 
        Parameters
        ----------
        expId : `int`
            Exposure ID.
 
        expBits : `int`
            Number of used bits in ``expId``.
 
        Returns
        -------
        idFactory : `lsst.afw.table.IdFactory`
            Generator object to assign ids to detected sources in the difference image.
 
        Notes
        -----
        The diasource id-s consists of the ``expId`` stored fixed in the highest value
        ``expBits`` of the 64-bit integer plus (bitwise or) a generated sequence number in the
        low value end of the integer.
        """
        return ExposureIdInfo(expId, expBits).makeSourceIdFactory()
 
    @lsst.utils.inheritDoc(pipeBase.PipelineTask)
    def runQuantum(self, butlerQC: pipeBase.ButlerQuantumContext,
                   inputRefs: pipeBase.InputQuantizedConnection,
                   outputRefs: pipeBase.OutputQuantizedConnection):
        inputs = butlerQC.get(inputRefs)
        self.log.info("Processing %s", butlerQC.quantum.dataId)
 
        finalizedPsfApCorrCatalog = inputs.get("finalizedPsfApCorrCatalog", None)
        exposure = self.prepareCalibratedExposure(
            inputs["exposure"],
            finalizedPsfApCorrCatalog=finalizedPsfApCorrCatalog
        )
 
        expId, expBits = butlerQC.quantum.dataId.pack("visit_detector",
                                                      returnMaxBits=True)
        idFactory = self.makeIdFactory(expId=expId, expBits=expBits)
        if self.config.coaddName == 'dcr':
            templateExposures = inputRefs.dcrCoadds
        else:
            templateExposures = inputRefs.coaddExposures
        templateStruct = self.getTemplate.runQuantum(
            exposure, butlerQC, inputRefs.skyMap, templateExposures
        )
 
        self.checkTemplateIsSufficient(templateStruct.exposure)
 
        outputs = self.run(exposure=exposure,
                           templateExposure=templateStruct.exposure,
                           idFactory=idFactory)
        # Consistency with runDataref gen2 handling
        if outputs.diaSources is None:
            del outputs.diaSources
        butlerQC.put(outputs, outputRefs)
 
    def prepareCalibratedExposure(self, exposure, finalizedPsfApCorrCatalog=None):
        """Prepare a calibrated exposure and apply finalized psf if so configured.
 
        Parameters
        ----------
        exposure : `lsst.afw.image.exposure.Exposure`
            Input exposure to adjust calibrations.
        finalizedPsfApCorrCatalog : `lsst.afw.table.ExposureCatalog`, optional
            Exposure catalog with finalized psf models and aperture correction
            maps to be applied if config.doApplyFinalizedPsf=True.  Catalog uses
            the detector id for the catalog id, sorted on id for fast lookup.
 
        Returns
        -------
        exposure : `lsst.afw.image.exposure.Exposure`
            Exposure with adjusted calibrations.
        """
        detectorId = exposure.getInfo().getDetector().getId()
 
        if finalizedPsfApCorrCatalog is not None:
            row = finalizedPsfApCorrCatalog.find(detectorId)
            if row is None:
                self.log.warning("Detector id %s not found in finalizedPsfApCorrCatalog; "
                                 "Using original psf.", detectorId)
            else:
                psf = row.getPsf()
                apCorrMap = row.getApCorrMap()
                if psf is None or apCorrMap is None:
                    self.log.warning("Detector id %s has None for psf/apCorrMap in "
                                     "finalizedPsfApCorrCatalog; Using original psf.", detectorId)
                else:
                    exposure.setPsf(psf)
                    exposure.info.setApCorrMap(apCorrMap)
 
        return exposure
 
    @timeMethod
    def run(self, exposure=None, selectSources=None, templateExposure=None, templateSources=None,
            idFactory=None, calexpBackgroundExposure=None, subtractedExposure=None):
        """PSF matches, subtract two images and perform detection on the difference image.
 
        Parameters
        ----------
        exposure : `lsst.afw.image.ExposureF`, optional
            The science exposure, the minuend in the image subtraction.
            Can be None only if ``config.doSubtract==False``.
        selectSources : `lsst.afw.table.SourceCatalog`, optional
            Identified sources on the science exposure. This catalog is used to
            select sources in order to perform the AL PSF matching on stamp images
            around them. The selection steps depend on config options and whether
            ``templateSources`` and ``matchingSources`` specified.
        templateExposure : `lsst.afw.image.ExposureF`, optional
            The template to be subtracted from ``exposure`` in the image subtraction.
            ``templateExposure`` is modified in place if ``config.doScaleTemplateVariance==True``.
            The template exposure should cover the same sky area as the science exposure.
            It is either a stich of patches of a coadd skymap image or a calexp
            of the same pointing as the science exposure. Can be None only
            if ``config.doSubtract==False`` and ``subtractedExposure`` is not None.
        templateSources : `lsst.afw.table.SourceCatalog`, optional
            Identified sources on the template exposure.
        idFactory : `lsst.afw.table.IdFactory`
            Generator object to assign ids to detected sources in the difference image.
        calexpBackgroundExposure : `lsst.afw.image.ExposureF`, optional
            Background exposure to be added back to the science exposure
            if ``config.doAddCalexpBackground==True``.
        subtractedExposure : `lsst.afw.image.ExposureF`, optional
            If ``config.doSubtract==False`` and ``config.doDetection==True``,
            performs the post subtraction source detection only on this exposure.
            Otherwise should be None.
 
        Returns
        -------
        results : `lsst.pipe.base.Struct`
            Results as a struct with attributes:
 
            ``subtractedExposure``
                Difference image (`lsst.afw.image.ExposureF`).
            ``scoreExposure``
                The zogy score exposure, if calculated (`lsst.afw.image.ExposureF` or `None`).
            ``matchedExposure``
                The matched PSF exposure (`lsst.afw.image.ExposureF`).
            ``subtractRes``
                The returned result structure of the ImagePsfMatchTask subtask (`lsst.pipe.base.Struct`).
            ``diaSources``
                The catalog of detected sources (`lsst.afw.table.SourceCatalog`).
            ``selectSources``
                The input source catalog with optionally added Qa information
                (`lsst.afw.table.SourceCatalog`).
 
        Notes
        -----
        The following major steps are included:
 
        - warp template coadd to match WCS of image
        - PSF match image to warped template
        - subtract image from PSF-matched, warped template
        - detect sources
        - measure sources
 
        For details about the image subtraction configuration modes
        see `lsst.ip.diffim`.
        """
        subtractRes = None
        controlSources = None
        subtractedExposure = None
        scoreExposure = None
        diaSources = None
        kernelSources = None
        # We'll clone exposure if modified but will still need the original
        exposureOrig = exposure
 
        if self.config.doAddCalexpBackground:
            mi = exposure.getMaskedImage()
            mi += calexpBackgroundExposure.getImage()
 
        if not exposure.hasPsf():
            raise pipeBase.TaskError("Exposure has no psf")
        sciencePsf = exposure.getPsf()
 
        if self.config.doSubtract:
            if self.config.doScaleTemplateVariance:
                self.log.info("Rescaling template variance")
                templateVarFactor = self.scaleVariance.run(
                    templateExposure.getMaskedImage())
                self.log.info("Template variance scaling factor: %.2f", templateVarFactor)
                self.metadata.add("scaleTemplateVarianceFactor", templateVarFactor)
            self.metadata.add("psfMatchingAlgorithm", self.config.subtract.name)
 
            if self.config.subtract.name == 'zogy':
                subtractRes = self.subtract.run(exposure, templateExposure, doWarping=True)
                scoreExposure = subtractRes.scoreExp
                subtractedExposure = subtractRes.diffExp
                subtractRes.subtractedExposure = subtractedExposure
                subtractRes.matchedExposure = None
 
            elif self.config.subtract.name == 'al':
                # compute scienceSigmaOrig: sigma of PSF of science image before pre-convolution
                # Just need a rough estimate; average positions are fine
                sciAvgPos = sciencePsf.getAveragePosition()
                scienceSigmaOrig = sciencePsf.computeShape(sciAvgPos).getDeterminantRadius()
 
                templatePsf = templateExposure.getPsf()
                templateAvgPos = templatePsf.getAveragePosition()
                templateSigma = templatePsf.computeShape(templateAvgPos).getDeterminantRadius()
 
                # if requested, convolve the science exposure with its PSF
                # (properly, this should be a cross-correlation, but our code does not yet support that)
                # compute scienceSigmaPost: sigma of science exposure with pre-convolution, if done,
                # else sigma of original science exposure
                # TODO: DM-22762 This functional block should be moved into its own method
                preConvPsf = None
                if self.config.useScoreImageDetection:
                    self.log.warning("AL likelihood image: pre-convolution of PSF is not implemented.")
                    convControl = afwMath.ConvolutionControl()
                    # cannot convolve in place, so need a new image anyway
                    srcMI = exposure.maskedImage
                    exposure = exposure.clone()  # New deep copy
                    srcPsf = sciencePsf
                    if self.config.useGaussianForPreConvolution:
                        self.log.info(
                            "AL likelihood image: Using Gaussian (sigma=%.2f) PSF estimation "
                            "for science image pre-convolution", scienceSigmaOrig)
                        # convolve with a simplified PSF model: a double Gaussian
                        kWidth, kHeight = sciencePsf.getLocalKernel(
                            sciencePsf.getAveragePosition()
                        ).getDimensions()
                        preConvPsf = SingleGaussianPsf(kWidth, kHeight, scienceSigmaOrig)
                    else:
                        # convolve with science exposure's PSF model
                        self.log.info(
                            "AL likelihood image: Using the science image PSF for pre-convolution.")
                        preConvPsf = srcPsf
                    afwMath.convolve(
                        exposure.maskedImage,
                        srcMI,
                        preConvPsf.getLocalKernel(preConvPsf.getAveragePosition()),
                        convControl
                    )
                    scienceSigmaPost = scienceSigmaOrig*math.sqrt(2)
                else:
                    scienceSigmaPost = scienceSigmaOrig
 
                # If requested, find and select sources from the image
                # else, AL subtraction will do its own source detection
                # TODO: DM-22762 This functional block should be moved into its own method
                if self.config.doSelectSources:
                    if selectSources is None:
                        self.log.warning("Src product does not exist; running detection, measurement,"
                                         " selection")
                        # Run own detection and measurement; necessary in nightly processing
                        selectSources = self.subtract.getSelectSources(
                            exposure,
                            sigma=scienceSigmaPost,
                            doSmooth=not self.config.useScoreImageDetection,
                            idFactory=idFactory,
                        )
 
                    if self.config.doAddMetrics:
                        # Number of basis functions
 
                        nparam = len(makeKernelBasisList(self.subtract.config.kernel.active,
                                                         referenceFwhmPix=scienceSigmaPost*FwhmPerSigma,
                                                         targetFwhmPix=templateSigma*FwhmPerSigma))
                        # Modify the schema of all Sources
                        # DEPRECATED: This is a data dependent (nparam) output product schema
                        # outside the task constructor.
                        # NOTE: The pre-determination of nparam at this point
                        # may be incorrect as the template psf is warped later in
                        # ImagePsfMatchTask.matchExposures()
                        kcQa = KernelCandidateQa(nparam)
                        selectSources = kcQa.addToSchema(selectSources)
                    if self.config.kernelSourcesFromRef:
                        # match exposure sources to reference catalog
                        astromRet = self.astrometer.loadAndMatch(exposure=exposure, sourceCat=selectSources)
                        matches = astromRet.matches
                    elif templateSources:
                        # match exposure sources to template sources
                        mc = afwTable.MatchControl()
                        mc.findOnlyClosest = False
                        matches = afwTable.matchRaDec(templateSources, selectSources, 1.0*geom.arcseconds,
                                                      mc)
                    else:
                        raise RuntimeError("doSelectSources=True and kernelSourcesFromRef=False,"
                                           "but template sources not available. Cannot match science "
                                           "sources with template sources. Run process* on data from "
                                           "which templates are built.")
 
                    kernelSources = self.sourceSelector.run(selectSources, exposure=exposure,
                                                            matches=matches).sourceCat
                    random.shuffle(kernelSources, random.random)
                    controlSources = kernelSources[::self.config.controlStepSize]
                    kernelSources = [k for i, k in enumerate(kernelSources)
                                     if i % self.config.controlStepSize]
 
                    if self.config.doSelectDcrCatalog:
                        redSelector = DiaCatalogSourceSelectorTask(
                            DiaCatalogSourceSelectorConfig(grMin=self.sourceSelector.config.grMax,
                                                           grMax=99.999))
                        redSources = redSelector.selectStars(exposure, selectSources, matches=matches).starCat
                        controlSources.extend(redSources)
 
                        blueSelector = DiaCatalogSourceSelectorTask(
                            DiaCatalogSourceSelectorConfig(grMin=-99.999,
                                                           grMax=self.sourceSelector.config.grMin))
                        blueSources = blueSelector.selectStars(exposure, selectSources,
                                                               matches=matches).starCat
                        controlSources.extend(blueSources)
 
                    if self.config.doSelectVariableCatalog:
                        varSelector = DiaCatalogSourceSelectorTask(
                            DiaCatalogSourceSelectorConfig(includeVariable=True))
                        varSources = varSelector.selectStars(exposure, selectSources, matches=matches).starCat
                        controlSources.extend(varSources)
 
                    self.log.info("Selected %d / %d sources for Psf matching (%d for control sample)",
                                  len(kernelSources), len(selectSources), len(controlSources))
 
                allresids = {}
                # TODO: DM-22762 This functional block should be moved into its own method
                if self.config.doUseRegister:
                    self.log.info("Registering images")
 
                    if templateSources is None:
                        # Run detection on the template, which is
                        # temporarily background-subtracted
                        # sigma of PSF of template image before warping
                        templateSources = self.subtract.getSelectSources(
                            templateExposure,
                            sigma=templateSigma,
                            doSmooth=True,
                            idFactory=idFactory
                        )
 
                    # Third step: we need to fit the relative astrometry.
                    #
                    wcsResults = self.fitAstrometry(templateSources, templateExposure, selectSources)
                    warpedExp = self.register.warpExposure(templateExposure, wcsResults.wcs,
                                                           exposure.getWcs(), exposure.getBBox())
                    templateExposure = warpedExp
 
                    # Create debugging outputs on the astrometric
                    # residuals as a function of position.  Persistence
                    # not yet implemented; expected on (I believe) #2636.
                    if self.config.doDebugRegister:
                        # Grab matches to reference catalog
                        srcToMatch = {x.second.getId(): x.first for x in matches}
 
                        refCoordKey = wcsResults.matches[0].first.getTable().getCoordKey()
                        inCentroidKey = wcsResults.matches[0].second.getTable().getCentroidSlot().getMeasKey()
                        sids = [m.first.getId() for m in wcsResults.matches]
                        positions = [m.first.get(refCoordKey) for m in wcsResults.matches]
                        residuals = [m.first.get(refCoordKey).getOffsetFrom(wcsResults.wcs.pixelToSky(
                            m.second.get(inCentroidKey))) for m in wcsResults.matches]
                        allresids = dict(zip(sids, zip(positions, residuals)))
 
                        cresiduals = [m.first.get(refCoordKey).getTangentPlaneOffset(
                            wcsResults.wcs.pixelToSky(
                                m.second.get(inCentroidKey))) for m in wcsResults.matches]
                        colors = numpy.array([-2.5*numpy.log10(srcToMatch[x].get("g"))
                                              + 2.5*numpy.log10(srcToMatch[x].get("r"))
                                              for x in sids if x in srcToMatch.keys()])
                        dlong = numpy.array([r[0].asArcseconds() for s, r in zip(sids, cresiduals)
                                             if s in srcToMatch.keys()])
                        dlat = numpy.array([r[1].asArcseconds() for s, r in zip(sids, cresiduals)
                                            if s in srcToMatch.keys()])
                        idx1 = numpy.where(colors < self.sourceSelector.config.grMin)
                        idx2 = numpy.where((colors >= self.sourceSelector.config.grMin)
                                           & (colors <= self.sourceSelector.config.grMax))
                        idx3 = numpy.where(colors > self.sourceSelector.config.grMax)
                        rms1Long = IqrToSigma*(
                            (numpy.percentile(dlong[idx1], 75) - numpy.percentile(dlong[idx1], 25)))
                        rms1Lat = IqrToSigma*(numpy.percentile(dlat[idx1], 75)
                                              - numpy.percentile(dlat[idx1], 25))
                        rms2Long = IqrToSigma*(
                            (numpy.percentile(dlong[idx2], 75) - numpy.percentile(dlong[idx2], 25)))
                        rms2Lat = IqrToSigma*(numpy.percentile(dlat[idx2], 75)
                                              - numpy.percentile(dlat[idx2], 25))
                        rms3Long = IqrToSigma*(
                            (numpy.percentile(dlong[idx3], 75) - numpy.percentile(dlong[idx3], 25)))
                        rms3Lat = IqrToSigma*(numpy.percentile(dlat[idx3], 75)
                                              - numpy.percentile(dlat[idx3], 25))
                        self.log.info("Blue star offsets'': %.3f %.3f, %.3f %.3f",
                                      numpy.median(dlong[idx1]), rms1Long,
                                      numpy.median(dlat[idx1]), rms1Lat)
                        self.log.info("Green star offsets'': %.3f %.3f, %.3f %.3f",
                                      numpy.median(dlong[idx2]), rms2Long,
                                      numpy.median(dlat[idx2]), rms2Lat)
                        self.log.info("Red star offsets'': %.3f %.3f, %.3f %.3f",
                                      numpy.median(dlong[idx3]), rms3Long,
                                      numpy.median(dlat[idx3]), rms3Lat)
 
                        self.metadata.add("RegisterBlueLongOffsetMedian", numpy.median(dlong[idx1]))
                        self.metadata.add("RegisterGreenLongOffsetMedian", numpy.median(dlong[idx2]))
                        self.metadata.add("RegisterRedLongOffsetMedian", numpy.median(dlong[idx3]))
                        self.metadata.add("RegisterBlueLongOffsetStd", rms1Long)
                        self.metadata.add("RegisterGreenLongOffsetStd", rms2Long)
                        self.metadata.add("RegisterRedLongOffsetStd", rms3Long)
 
                        self.metadata.add("RegisterBlueLatOffsetMedian", numpy.median(dlat[idx1]))
                        self.metadata.add("RegisterGreenLatOffsetMedian", numpy.median(dlat[idx2]))
                        self.metadata.add("RegisterRedLatOffsetMedian", numpy.median(dlat[idx3]))
                        self.metadata.add("RegisterBlueLatOffsetStd", rms1Lat)
                        self.metadata.add("RegisterGreenLatOffsetStd", rms2Lat)
                        self.metadata.add("RegisterRedLatOffsetStd", rms3Lat)
 
                # warp template exposure to match exposure,
                # PSF match template exposure to exposure,
                # then return the difference
 
                # Return warped template...  Construct sourceKernelCand list after subtract
                self.log.info("Subtracting images")
                subtractRes = self.subtract.subtractExposures(
                    templateExposure=templateExposure,
                    scienceExposure=exposure,
                    candidateList=kernelSources,
                    convolveTemplate=self.config.convolveTemplate,
                    doWarping=not self.config.doUseRegister
                )
                if self.config.useScoreImageDetection:
                    scoreExposure = subtractRes.subtractedExposure
                else:
                    subtractedExposure = subtractRes.subtractedExposure
 
                if self.config.doDetection:
                    self.log.info("Computing diffim PSF")
 
                    # Get Psf from the appropriate input image if it doesn't exist
                    if subtractedExposure is not None and not subtractedExposure.hasPsf():
                        if self.config.convolveTemplate:
                            subtractedExposure.setPsf(exposure.getPsf())
                        else:
                            subtractedExposure.setPsf(templateExposure.getPsf())
 
                # If doSubtract is False, then subtractedExposure was fetched from disk (above),
                # thus it may have already been decorrelated. Thus, we do not decorrelate if
                # doSubtract is False.
 
                # NOTE: At this point doSubtract == True
                if self.config.doDecorrelation and self.config.doSubtract:
                    preConvKernel = None
                    if self.config.useGaussianForPreConvolution:
                        preConvKernel = preConvPsf.getLocalKernel(preConvPsf.getAveragePosition())
                    if self.config.useScoreImageDetection:
                        scoreExposure = self.decorrelate.run(exposureOrig, subtractRes.warpedExposure,
                                                             scoreExposure,
                                                             subtractRes.psfMatchingKernel,
                                                             spatiallyVarying=self.config.doSpatiallyVarying,
                                                             preConvKernel=preConvKernel,
                                                             templateMatched=True,
                                                             preConvMode=True).correctedExposure
                    # Note that the subtracted exposure is always decorrelated,
                    # even if the score image is used for detection
                    subtractedExposure = self.decorrelate.run(exposureOrig, subtractRes.warpedExposure,
                                                              subtractedExposure,
                                                              subtractRes.psfMatchingKernel,
                                                              spatiallyVarying=self.config.doSpatiallyVarying,
                                                              preConvKernel=None,
                                                              templateMatched=self.config.convolveTemplate,
                                                              preConvMode=False).correctedExposure
            # END (if subtractAlgorithm == 'AL')
        # END (if self.config.doSubtract)
        if self.config.doDetection:
            self.log.info("Running diaSource detection")
 
            # subtractedExposure - reserved for task return value
            # in zogy, it is always the proper difference image
            # in AL, it may be (yet) pre-convolved and/or decorrelated
            #
            # detectionExposure - controls which exposure to use for detection
            # in-place modifications will appear in task return
            if self.config.useScoreImageDetection:
                # zogy with score image detection enabled
                self.log.info("Detection, diffim rescaling and measurements are "
                              "on AL likelihood or Zogy score image.")
                detectionExposure = scoreExposure
            else:
                # AL or zogy with no score image detection
                detectionExposure = subtractedExposure
 
            # Rescale difference image variance plane
            if self.config.doScaleDiffimVariance:
                self.log.info("Rescaling diffim variance")
                diffimVarFactor = self.scaleVariance.run(detectionExposure.getMaskedImage())
                self.log.info("Diffim variance scaling factor: %.2f", diffimVarFactor)
                self.metadata.add("scaleDiffimVarianceFactor", diffimVarFactor)
 
            # Erase existing detection mask planes
            mask = detectionExposure.getMaskedImage().getMask()
            mask &= ~(mask.getPlaneBitMask("DETECTED") | mask.getPlaneBitMask("DETECTED_NEGATIVE"))
 
            table = afwTable.SourceTable.make(self.schema, idFactory)
            table.setMetadata(self.algMetadata)
            results = self.detection.run(
                table=table,
                exposure=detectionExposure,
                doSmooth=not self.config.useScoreImageDetection
            )
 
            if self.config.doMerge:
                fpSet = results.fpSets.positive
                fpSet.merge(results.fpSets.negative, self.config.growFootprint,
                            self.config.growFootprint, False)
                diaSources = afwTable.SourceCatalog(table)
                fpSet.makeSources(diaSources)
                self.log.info("Merging detections into %d sources", len(diaSources))
            else:
                diaSources = results.sources
            # Inject skySources before measurement.
            if self.config.doSkySources:
                skySourceFootprints = self.skySources.run(
                    mask=detectionExposure.mask,
                    seed=detectionExposure.info.id)
                if skySourceFootprints:
                    for foot in skySourceFootprints:
                        s = diaSources.addNew()
                        s.setFootprint(foot)
                        s.set(self.skySourceKey, True)
 
            if self.config.doMeasurement:
                newDipoleFitting = self.config.doDipoleFitting
                self.log.info("Running diaSource measurement: newDipoleFitting=%r", newDipoleFitting)
                if not newDipoleFitting:
                    # Just fit dipole in diffim
                    self.measurement.run(diaSources, detectionExposure)
                else:
                    # Use (matched) template and science image (if avail.) to constrain dipole fitting
                    if self.config.doSubtract and 'matchedExposure' in subtractRes.getDict():
                        self.measurement.run(diaSources, detectionExposure, exposure,
                                             subtractRes.matchedExposure)
                    else:
                        self.measurement.run(diaSources, detectionExposure, exposure)
                if self.config.doApCorr:
                    self.applyApCorr.run(
                        catalog=diaSources,
                        apCorrMap=detectionExposure.getInfo().getApCorrMap()
                    )
 
            if self.config.doForcedMeasurement:
                # Run forced psf photometry on the PVI at the diaSource locations.
                # Copy the measured flux and error into the diaSource.
                forcedSources = self.forcedMeasurement.generateMeasCat(
                    exposure, diaSources, detectionExposure.getWcs())
                self.forcedMeasurement.run(forcedSources, exposure, diaSources, detectionExposure.getWcs())
                mapper = afwTable.SchemaMapper(forcedSources.schema, diaSources.schema)
                mapper.addMapping(forcedSources.schema.find("base_PsfFlux_instFlux")[0],
                                  "ip_diffim_forced_PsfFlux_instFlux", True)
                mapper.addMapping(forcedSources.schema.find("base_PsfFlux_instFluxErr")[0],
                                  "ip_diffim_forced_PsfFlux_instFluxErr", True)
                mapper.addMapping(forcedSources.schema.find("base_PsfFlux_area")[0],
                                  "ip_diffim_forced_PsfFlux_area", True)
                mapper.addMapping(forcedSources.schema.find("base_PsfFlux_flag")[0],
                                  "ip_diffim_forced_PsfFlux_flag", True)
                mapper.addMapping(forcedSources.schema.find("base_PsfFlux_flag_noGoodPixels")[0],
                                  "ip_diffim_forced_PsfFlux_flag_noGoodPixels", True)
                mapper.addMapping(forcedSources.schema.find("base_PsfFlux_flag_edge")[0],
                                  "ip_diffim_forced_PsfFlux_flag_edge", True)
                for diaSource, forcedSource in zip(diaSources, forcedSources):
                    diaSource.assign(forcedSource, mapper)
 
            # Match with the calexp sources if possible
            if self.config.doMatchSources:
                if selectSources is not None:
                    # Create key,val pair where key=diaSourceId and val=sourceId
                    matchRadAsec = self.config.diaSourceMatchRadius
                    matchRadPixel = matchRadAsec/exposure.getWcs().getPixelScale().asArcseconds()
 
                    srcMatches = afwTable.matchXy(selectSources, diaSources, matchRadPixel)
                    srcMatchDict = dict([(srcMatch.second.getId(), srcMatch.first.getId()) for
                                         srcMatch in srcMatches])
                    self.log.info("Matched %d / %d diaSources to sources",
                                  len(srcMatchDict), len(diaSources))
                else:
                    self.log.warning("Src product does not exist; cannot match with diaSources")
                    srcMatchDict = {}
 
                # Create key,val pair where key=diaSourceId and val=refId
                refAstromConfig = AstrometryConfig()
                refAstromConfig.matcher.maxMatchDistArcSec = matchRadAsec
                refAstrometer = AstrometryTask(self.refObjLoader, config=refAstromConfig)
                astromRet = refAstrometer.run(exposure=exposure, sourceCat=diaSources)
                refMatches = astromRet.matches
                if refMatches is None:
                    self.log.warning("No diaSource matches with reference catalog")
                    refMatchDict = {}
                else:
                    self.log.info("Matched %d / %d diaSources to reference catalog",
                                  len(refMatches), len(diaSources))
                    refMatchDict = dict([(refMatch.second.getId(), refMatch.first.getId()) for
                                         refMatch in refMatches])
 
                # Assign source Ids
                for diaSource in diaSources:
                    sid = diaSource.getId()
                    if sid in srcMatchDict:
                        diaSource.set("srcMatchId", srcMatchDict[sid])
                    if sid in refMatchDict:
                        diaSource.set("refMatchId", refMatchDict[sid])
 
            if self.config.doAddMetrics and self.config.doSelectSources:
                self.log.info("Evaluating metrics and control sample")
 
                kernelCandList = []
                for cell in subtractRes.kernelCellSet.getCellList():
                    for cand in cell.begin(False):  # include bad candidates
                        kernelCandList.append(cand)
 
                # Get basis list to build control sample kernels
                basisList = kernelCandList[0].getKernel(KernelCandidateF.ORIG).getKernelList()
                nparam = len(kernelCandList[0].getKernel(KernelCandidateF.ORIG).getKernelParameters())
 
                controlCandList = (
                    diffimTools.sourceTableToCandidateList(controlSources,
                                                           subtractRes.warpedExposure, exposure,
                                                           self.config.subtract.kernel.active,
                                                           self.config.subtract.kernel.active.detectionConfig,
                                                           self.log, doBuild=True, basisList=basisList))
 
                KernelCandidateQa.apply(kernelCandList, subtractRes.psfMatchingKernel,
                                        subtractRes.backgroundModel, dof=nparam)
                KernelCandidateQa.apply(controlCandList, subtractRes.psfMatchingKernel,
                                        subtractRes.backgroundModel)
 
                if self.config.doDetection:
                    KernelCandidateQa.aggregate(selectSources, self.metadata, allresids, diaSources)
                else:
                    KernelCandidateQa.aggregate(selectSources, self.metadata, allresids)
 
        self.runDebug(exposure, subtractRes, selectSources, kernelSources, diaSources)
        return pipeBase.Struct(
            subtractedExposure=subtractedExposure,
            scoreExposure=scoreExposure,
            warpedExposure=subtractRes.warpedExposure,
            matchedExposure=subtractRes.matchedExposure,
            subtractRes=subtractRes,
            diaSources=diaSources,
            selectSources=selectSources
        )
 
    def fitAstrometry(self, templateSources, templateExposure, selectSources):
        """Fit the relative astrometry between templateSources and selectSources
 
        Notes
        -----
        TODO: Remove this method. It originally fit a new WCS to the template before calling register.run
        because our TAN-SIP fitter behaved badly for points far from CRPIX, but that's been fixed.
        It remains because a subtask overrides it.
        """
        results = self.register.run(templateSources, templateExposure.getWcs(),
                                    templateExposure.getBBox(), selectSources)
        return results
 
    def runDebug(self, exposure, subtractRes, selectSources, kernelSources, diaSources):
        """Make debug plots and displays.
 
        Parameters
        ----------
        exposure : `lsst.afw.image.exposure.Exposure`
            Input exposure.
        subtractRes : `lsst.pipe.base.Struct`
            Returned result structure of the ImagePsfMatchTask subtask.
        selectSources : `lsst.afw.table.SourceCatalog`
            Input source catalog.
        kernelSources : `lsst.afw.table.SourceCatalog`
            unknown
        diaSources : `lsst.afw.table.SourceCatalog`
            The catalog of detected sources.
 
        Notes
        -----
        TODO: Test and update for current debug display and slot names.
        """
        import lsstDebug
        display = lsstDebug.Info(__name__).display
        showSubtracted = lsstDebug.Info(__name__).showSubtracted
        showPixelResiduals = lsstDebug.Info(__name__).showPixelResiduals
        showDiaSources = lsstDebug.Info(__name__).showDiaSources
        showDipoles = lsstDebug.Info(__name__).showDipoles
        maskTransparency = lsstDebug.Info(__name__).maskTransparency
        if display:
            disp = afwDisplay.getDisplay(frame=lsstDebug.frame)
            if not maskTransparency:
                maskTransparency = 0
            disp.setMaskTransparency(maskTransparency)
 
        if display and showSubtracted:
            disp.mtv(subtractRes.subtractedExposure, title="Subtracted image")
            mi = subtractRes.subtractedExposure.getMaskedImage()
            x0, y0 = mi.getX0(), mi.getY0()
            with disp.Buffering():
                for s in diaSources:
                    x, y = s.getX() - x0, s.getY() - y0
                    ctype = "red" if s.get("flags_negative") else "yellow"
                    if (s.get("base_PixelFlags_flag_interpolatedCenter")
                            or s.get("base_PixelFlags_flag_saturatedCenter")
                            or s.get("base_PixelFlags_flag_crCenter")):
                        ptype = "x"
                    elif (s.get("base_PixelFlags_flag_interpolated")
                          or s.get("base_PixelFlags_flag_saturated")
                          or s.get("base_PixelFlags_flag_cr")):
                        ptype = "+"
                    else:
                        ptype = "o"
                    disp.dot(ptype, x, y, size=4, ctype=ctype)
            lsstDebug.frame += 1
 
        if display and showPixelResiduals and selectSources:
            nonKernelSources = []
            for source in selectSources:
                if source not in kernelSources:
                    nonKernelSources.append(source)
 
            diUtils.plotPixelResiduals(exposure,
                                       subtractRes.warpedExposure,
                                       subtractRes.subtractedExposure,
                                       subtractRes.kernelCellSet,
                                       subtractRes.psfMatchingKernel,
                                       subtractRes.backgroundModel,
                                       nonKernelSources,
                                       self.subtract.config.kernel.active.detectionConfig,
                                       origVariance=False)
            diUtils.plotPixelResiduals(exposure,
                                       subtractRes.warpedExposure,
                                       subtractRes.subtractedExposure,
                                       subtractRes.kernelCellSet,
                                       subtractRes.psfMatchingKernel,
                                       subtractRes.backgroundModel,
                                       nonKernelSources,
                                       self.subtract.config.kernel.active.detectionConfig,
                                       origVariance=True)
        if display and showDiaSources:
            flagChecker = SourceFlagChecker(diaSources)
            isFlagged = [flagChecker(x) for x in diaSources]
            isDipole = [x.get("ip_diffim_ClassificationDipole_value") for x in diaSources]
            diUtils.showDiaSources(diaSources, subtractRes.subtractedExposure, isFlagged, isDipole,
                                   frame=lsstDebug.frame)
            lsstDebug.frame += 1
 
        if display and showDipoles:
            DipoleAnalysis().displayDipoles(subtractRes.subtractedExposure, diaSources,
                                            frame=lsstDebug.frame)
            lsstDebug.frame += 1
 
    def checkTemplateIsSufficient(self, templateExposure):
        """Raise NoWorkFound if template coverage < requiredTemplateFraction.
 
        Parameters
        ----------
        templateExposure : `lsst.afw.image.ExposureF`
            The template exposure to check.
 
        Raises
        ------
        NoWorkFound
            Raised if fraction of good pixels, defined as not having NO_DATA
            set, is less then the configured requiredTemplateFraction.
        """
        # Count the number of pixels with the NO_DATA mask bit set
        # counting NaN pixels is insufficient because pixels without data are often intepolated over)
        pixNoData = numpy.count_nonzero(templateExposure.mask.array
                                        & templateExposure.mask.getPlaneBitMask('NO_DATA'))
        pixGood = templateExposure.getBBox().getArea() - pixNoData
        self.log.info("template has %d good pixels (%.1f%%)", pixGood,
                      100*pixGood/templateExposure.getBBox().getArea())
 
        if pixGood/templateExposure.getBBox().getArea() < self.config.requiredTemplateFraction:
            message = ("Insufficient Template Coverage. (%.1f%% < %.1f%%) Not attempting subtraction. "
                       "To force subtraction, set config requiredTemplateFraction=0." % (
                           100*pixGood/templateExposure.getBBox().getArea(),
                           100*self.config.requiredTemplateFraction))
            raise pipeBase.NoWorkFound(message)
 
 
class ImageDifferenceFromTemplateConnections(ImageDifferenceTaskConnections,
                                             defaultTemplates={"coaddName": "goodSeeing"}
                                             ):
    inputTemplate = pipeBase.connectionTypes.Input(
        doc=("Warped template produced by GetMultiTractCoaddTemplate"),
        dimensions=("instrument", "visit", "detector"),
        storageClass="ExposureF",
        name="{fakesType}{coaddName}Diff_templateExp{warpTypeSuffix}",
    )
 
    def __init__(self, *, config=None):
        super().__init__(config=config)
        # ImageDifferenceConnections will have removed one of these.
        # Make sure they're both gone, because no coadds are needed.
        if "coaddExposures" in self.inputs:
            self.inputs.remove("coaddExposures")
        if "dcrCoadds" in self.inputs:
            self.inputs.remove("dcrCoadds")
 
 
class ImageDifferenceFromTemplateConfig(ImageDifferenceConfig,
                                        pipelineConnections=ImageDifferenceFromTemplateConnections):
    pass
 
 
class ImageDifferenceFromTemplateTask(ImageDifferenceTask):
    ConfigClass = ImageDifferenceFromTemplateConfig
    _DefaultName = "imageDifference"
 
    @lsst.utils.inheritDoc(pipeBase.PipelineTask)
    def runQuantum(self, butlerQC, inputRefs, outputRefs):
        inputs = butlerQC.get(inputRefs)
        self.log.info("Processing %s", butlerQC.quantum.dataId)
        self.checkTemplateIsSufficient(inputs['inputTemplate'])
        expId, expBits = butlerQC.quantum.dataId.pack("visit_detector",
                                                      returnMaxBits=True)
        idFactory = self.makeIdFactory(expId=expId, expBits=expBits)
 
        finalizedPsfApCorrCatalog = inputs.get("finalizedPsfApCorrCatalog", None)
        exposure = self.prepareCalibratedExposure(
            inputs["exposure"],
            finalizedPsfApCorrCatalog=finalizedPsfApCorrCatalog
        )
 
        outputs = self.run(exposure=exposure,
                           templateExposure=inputs['inputTemplate'],
                           idFactory=idFactory)
 
        # Consistency with runDataref gen2 handling
        if outputs.diaSources is None:
            del outputs.diaSources
        butlerQC.put(outputs, outputRefs)