makeCoaddTempExp.py

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#
# LSST Data Management System
# Copyright 2008, 2009, 2010, 2011, 2012 LSST Corporation.
#
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# LSST Project (http://www.lsst.org/).
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import numpy
 
import lsst.pex.config as pexConfig
import lsst.daf.persistence as dafPersist
import lsst.afw.image as afwImage
import lsst.coadd.utils as coaddUtils
import lsst.pipe.base as pipeBase
import lsst.pipe.base.connectionTypes as cT
import lsst.log as log
import lsst.utils as utils
from lsst.meas.algorithms import CoaddPsf, CoaddPsfConfig
from .coaddBase import CoaddBaseTask, makeSkyInfo
from .warpAndPsfMatch import WarpAndPsfMatchTask
from .coaddHelpers import groupPatchExposures, getGroupDataRef
 
__all__ = ["MakeCoaddTempExpTask", "MakeWarpTask", "MakeWarpConfig"]
 
 
class MissingExposureError(Exception):
    """Raised when data cannot be retrieved for an exposure.
    When processing patches, sometimes one exposure is missing; this lets us
    distinguish bewteen that case, and other errors.
    """
    pass
 
 
class MakeCoaddTempExpConfig(CoaddBaseTask.ConfigClass):
    """Config for MakeCoaddTempExpTask
    """
    warpAndPsfMatch = pexConfig.ConfigurableField(
        target=WarpAndPsfMatchTask,
        doc="Task to warp and PSF-match calexp",
    )
    doWrite = pexConfig.Field(
        doc="persist <coaddName>Coadd_<warpType>Warp",
        dtype=bool,
        default=True,
    )
    bgSubtracted = pexConfig.Field(
        doc="Work with a background subtracted calexp?",
        dtype=bool,
        default=True,
    )
    coaddPsf = pexConfig.ConfigField(
        doc="Configuration for CoaddPsf",
        dtype=CoaddPsfConfig,
    )
    makeDirect = pexConfig.Field(
        doc="Make direct Warp/Coadds",
        dtype=bool,
        default=True,
    )
    makePsfMatched = pexConfig.Field(
        doc="Make Psf-Matched Warp/Coadd?",
        dtype=bool,
        default=False,
    )
 
    doWriteEmptyWarps = pexConfig.Field(
        dtype=bool,
        default=False,
        doc="Write out warps even if they are empty"
    )
 
    hasFakes = pexConfig.Field(
        doc="Should be set to True if fake sources have been inserted into the input data.",
        dtype=bool,
        default=False,
    )
    doApplySkyCorr = pexConfig.Field(dtype=bool, default=False, doc="Apply sky correction?")
 
    def validate(self):
        CoaddBaseTask.ConfigClass.validate(self)
        if not self.makePsfMatched and not self.makeDirect:
            raise RuntimeError("At least one of config.makePsfMatched and config.makeDirect must be True")
        if self.doPsfMatch:
            # Backwards compatibility.
            log.warn("Config doPsfMatch deprecated. Setting makePsfMatched=True and makeDirect=False")
            self.makePsfMatched = True
            self.makeDirect = False
 
    def setDefaults(self):
        CoaddBaseTask.ConfigClass.setDefaults(self)
        self.warpAndPsfMatch.psfMatch.kernel.active.kernelSize = self.matchingKernelSize
 
 
 
 
class MakeCoaddTempExpTask(CoaddBaseTask):
    r"""!Warp and optionally PSF-Match calexps onto an a common projection.
 
    @anchor MakeCoaddTempExpTask_
 
    @section pipe_tasks_makeCoaddTempExp_Contents  Contents
 
     - @ref pipe_tasks_makeCoaddTempExp_Purpose
     - @ref pipe_tasks_makeCoaddTempExp_Initialize
     - @ref pipe_tasks_makeCoaddTempExp_IO
     - @ref pipe_tasks_makeCoaddTempExp_Config
     - @ref pipe_tasks_makeCoaddTempExp_Debug
     - @ref pipe_tasks_makeCoaddTempExp_Example
 
    @section pipe_tasks_makeCoaddTempExp_Purpose  Description
 
    Warp and optionally PSF-Match calexps onto a common projection, by
    performing the following operations:
    - Group calexps by visit/run
    - For each visit, generate a Warp by calling method @ref makeTempExp.
      makeTempExp loops over the visit's calexps calling @ref WarpAndPsfMatch
      on each visit
 
    The result is a `directWarp` (and/or optionally a `psfMatchedWarp`).
 
    @section pipe_tasks_makeCoaddTempExp_Initialize  Task Initialization
 
    @copydoc \_\_init\_\_
 
    This task has one special keyword argument: passing reuse=True will cause
    the task to skip the creation of warps that are already present in the
    output repositories.
 
    @section pipe_tasks_makeCoaddTempExp_IO  Invoking the Task
 
    This task is primarily designed to be run from the command line.
 
    The main method is `runDataRef`, which takes a single butler data reference for the patch(es)
    to process.
 
    @copydoc run
 
    WarpType identifies the types of convolutions applied to Warps (previously CoaddTempExps).
    Only two types are available: direct (for regular Warps/Coadds) and psfMatched
    (for Warps/Coadds with homogenized PSFs). We expect to add a third type, likelihood,
    for generating likelihood Coadds with Warps that have been correlated with their own PSF.
 
    @section pipe_tasks_makeCoaddTempExp_Config  Configuration parameters
 
    See @ref MakeCoaddTempExpConfig and parameters inherited from
    @link lsst.pipe.tasks.coaddBase.CoaddBaseConfig CoaddBaseConfig @endlink
 
    @subsection pipe_tasks_MakeCoaddTempExp_psfMatching Guide to PSF-Matching Configs
 
    To make `psfMatchedWarps`, select `config.makePsfMatched=True`. The subtask
    @link lsst.ip.diffim.modelPsfMatch.ModelPsfMatchTask ModelPsfMatchTask @endlink
    is responsible for the PSF-Matching, and its config is accessed via `config.warpAndPsfMatch.psfMatch`.
    The optimal configuration depends on aspects of dataset: the pixel scale, average PSF FWHM and
    dimensions of the PSF kernel. These configs include the requested model PSF, the matching kernel size,
    padding of the science PSF thumbnail and spatial sampling frequency of the PSF.
 
    *Config Guidelines*: The user must specify the size of the model PSF to which to match by setting
    `config.modelPsf.defaultFwhm` in units of pixels. The appropriate values depends on science case.
    In general, for a set of input images, this config should equal the FWHM of the visit
    with the worst seeing. The smallest it should be set to is the median FWHM. The defaults
    of the other config options offer a reasonable starting point.
    The following list presents the most common problems that arise from a misconfigured
    @link lsst.ip.diffim.modelPsfMatch.ModelPsfMatchTask ModelPsfMatchTask @endlink
    and corresponding solutions. All assume the default Alard-Lupton kernel, with configs accessed via
    ```config.warpAndPsfMatch.psfMatch.kernel['AL']```. Each item in the list is formatted as:
    Problem: Explanation. *Solution*
 
    *Troublshooting PSF-Matching Configuration:*
    - Matched PSFs look boxy: The matching kernel is too small. _Increase the matching kernel size.
        For example:_
 
            config.warpAndPsfMatch.psfMatch.kernel['AL'].kernelSize=27  # default 21
 
        Note that increasing the kernel size also increases runtime.
    - Matched PSFs look ugly (dipoles, quadropoles, donuts): unable to find good solution
        for matching kernel. _Provide the matcher with more data by either increasing
        the spatial sampling by decreasing the spatial cell size,_
 
            config.warpAndPsfMatch.psfMatch.kernel['AL'].sizeCellX = 64  # default 128
            config.warpAndPsfMatch.psfMatch.kernel['AL'].sizeCellY = 64  # default 128
 
        _or increasing the padding around the Science PSF, for example:_
 
            config.warpAndPsfMatch.psfMatch.autoPadPsfTo=1.6  # default 1.4
 
        Increasing `autoPadPsfTo` increases the minimum ratio of input PSF dimensions to the
        matching kernel dimensions, thus increasing the number of pixels available to fit
        after convolving the PSF with the matching kernel.
        Optionally, for debugging the effects of padding, the level of padding may be manually
        controlled by setting turning off the automatic padding and setting the number
        of pixels by which to pad the PSF:
 
            config.warpAndPsfMatch.psfMatch.doAutoPadPsf = False  # default True
            config.warpAndPsfMatch.psfMatch.padPsfBy = 6  # pixels. default 0
 
    - Deconvolution: Matching a large PSF to a smaller PSF produces
        a telltale noise pattern which looks like ripples or a brain.
        _Increase the size of the requested model PSF. For example:_
 
            config.modelPsf.defaultFwhm = 11  # Gaussian sigma in units of pixels.
 
    - High frequency (sometimes checkered) noise: The matching basis functions are too small.
        _Increase the width of the Gaussian basis functions. For example:_
 
            config.warpAndPsfMatch.psfMatch.kernel['AL'].alardSigGauss=[1.5, 3.0, 6.0]
            # from default [0.7, 1.5, 3.0]
 
 
    @section pipe_tasks_makeCoaddTempExp_Debug  Debug variables
 
    MakeCoaddTempExpTask has no debug output, but its subtasks do.
 
    @section pipe_tasks_makeCoaddTempExp_Example   A complete example of using MakeCoaddTempExpTask
 
    This example uses the package ci_hsc to show how MakeCoaddTempExp fits
    into the larger Data Release Processing.
    Set up by running:
 
        setup ci_hsc
        cd $CI_HSC_DIR
        # if not built already:
        python $(which scons)  # this will take a while
 
    The following assumes that `processCcd.py` and `makeSkyMap.py` have previously been run
    (e.g. by building `ci_hsc` above) to generate a repository of calexps and an
    output respository with the desired SkyMap. The command,
 
        makeCoaddTempExp.py $CI_HSC_DIR/DATA --rerun ci_hsc \
         --id patch=5,4 tract=0 filter=HSC-I \
         --selectId visit=903988 ccd=16 --selectId visit=903988 ccd=17 \
         --selectId visit=903988 ccd=23 --selectId visit=903988 ccd=24 \
         --config doApplyExternalPhotoCalib=False doApplyExternalSkyWcs=False \
         makePsfMatched=True modelPsf.defaultFwhm=11
 
    writes a direct and PSF-Matched Warp to
    - `$CI_HSC_DIR/DATA/rerun/ci_hsc/deepCoadd/HSC-I/0/5,4/warp-HSC-I-0-5,4-903988.fits` and
    - `$CI_HSC_DIR/DATA/rerun/ci_hsc/deepCoadd/HSC-I/0/5,4/psfMatchedWarp-HSC-I-0-5,4-903988.fits`
        respectively.
 
    @note PSF-Matching in this particular dataset would benefit from adding
    `--configfile ./matchingConfig.py` to
    the command line arguments where `matchingConfig.py` is defined by:
 
        echo "
        config.warpAndPsfMatch.psfMatch.kernel['AL'].kernelSize=27
        config.warpAndPsfMatch.psfMatch.kernel['AL'].alardSigGauss=[1.5, 3.0, 6.0]" > matchingConfig.py
 
 
    Add the option `--help` to see more options.
    """
    ConfigClass = MakeCoaddTempExpConfig
    _DefaultName = "makeCoaddTempExp"
 
    def __init__(self, reuse=False, **kwargs):
        CoaddBaseTask.__init__(self, **kwargs)
        self.reuse = reuse
        self.makeSubtask("warpAndPsfMatch")
        if self.config.hasFakes:
            self.calexpType = "fakes_calexp"
        else:
            self.calexpType = "calexp"
 
    @pipeBase.timeMethod
    def runDataRef(self, patchRef, selectDataList=[]):
        """!Produce <coaddName>Coadd_<warpType>Warp images by warping and optionally PSF-matching.
 
        @param[in] patchRef: data reference for sky map patch. Must include keys "tract", "patch",
            plus the camera-specific filter key (e.g. "filter" or "band")
        @return: dataRefList: a list of data references for the new <coaddName>Coadd_directWarps
            if direct or both warp types are requested and <coaddName>Coadd_psfMatchedWarps if only psfMatched
            warps are requested.
 
        @warning: this task assumes that all exposures in a warp (coaddTempExp) have the same filter.
 
        @warning: this task sets the PhotoCalib of the coaddTempExp to the PhotoCalib of the first calexp
        with any good pixels in the patch. For a mosaic camera the resulting PhotoCalib should be ignored
        (assembleCoadd should determine zeropoint scaling without referring to it).
        """
        skyInfo = self.getSkyInfo(patchRef)
 
        # DataRefs to return are of type *_directWarp unless only *_psfMatchedWarp requested
        if self.config.makePsfMatched and not self.config.makeDirect:
            primaryWarpDataset = self.getTempExpDatasetName("psfMatched")
        else:
            primaryWarpDataset = self.getTempExpDatasetName("direct")
 
        calExpRefList = self.selectExposures(patchRef, skyInfo, selectDataList=selectDataList)
 
        if len(calExpRefList) == 0:
            self.log.warn("No exposures to coadd for patch %s", patchRef.dataId)
            return None
        self.log.info("Selected %d calexps for patch %s", len(calExpRefList), patchRef.dataId)
        calExpRefList = [calExpRef for calExpRef in calExpRefList if calExpRef.datasetExists(self.calexpType)]
        self.log.info("Processing %d existing calexps for patch %s", len(calExpRefList), patchRef.dataId)
 
        groupData = groupPatchExposures(patchRef, calExpRefList, self.getCoaddDatasetName(),
                                        primaryWarpDataset)
        self.log.info("Processing %d warp exposures for patch %s", len(groupData.groups), patchRef.dataId)
 
        dataRefList = []
        for i, (tempExpTuple, calexpRefList) in enumerate(groupData.groups.items()):
            tempExpRef = getGroupDataRef(patchRef.getButler(), primaryWarpDataset,
                                         tempExpTuple, groupData.keys)
            if self.reuse and tempExpRef.datasetExists(datasetType=primaryWarpDataset, write=True):
                self.log.info("Skipping makeCoaddTempExp for %s; output already exists.", tempExpRef.dataId)
                dataRefList.append(tempExpRef)
                continue
            self.log.info("Processing Warp %d/%d: id=%s", i, len(groupData.groups), tempExpRef.dataId)
 
            # TODO: mappers should define a way to go from the "grouping keys" to a numeric ID (#2776).
            # For now, we try to get a long integer "visit" key, and if we can't, we just use the index
            # of the visit in the list.
            try:
                visitId = int(tempExpRef.dataId["visit"])
            except (KeyError, ValueError):
                visitId = i
 
            calExpList = []
            ccdIdList = []
            dataIdList = []
 
            for calExpInd, calExpRef in enumerate(calexpRefList):
                self.log.info("Reading calexp %s of %s for Warp id=%s", calExpInd+1, len(calexpRefList),
                              calExpRef.dataId)
                try:
                    ccdId = calExpRef.get("ccdExposureId", immediate=True)
                except Exception:
                    ccdId = calExpInd
                try:
                    # We augment the dataRef here with the tract, which is harmless for loading things
                    # like calexps that don't need the tract, and necessary for meas_mosaic outputs,
                    # which do.
                    calExpRef = calExpRef.butlerSubset.butler.dataRef(self.calexpType,
                                                                      dataId=calExpRef.dataId,
                                                                      tract=skyInfo.tractInfo.getId())
                    calExp = self.getCalibratedExposure(calExpRef, bgSubtracted=self.config.bgSubtracted)
                except Exception as e:
                    self.log.warn("Calexp %s not found; skipping it: %s", calExpRef.dataId, e)
                    continue
 
                if self.config.doApplySkyCorr:
                    self.applySkyCorr(calExpRef, calExp)
 
                calExpList.append(calExp)
                ccdIdList.append(ccdId)
                dataIdList.append(calExpRef.dataId)
 
            exps = self.run(calExpList, ccdIdList, skyInfo, visitId, dataIdList).exposures
 
            if any(exps.values()):
                dataRefList.append(tempExpRef)
            else:
                self.log.warn("Warp %s could not be created", tempExpRef.dataId)
 
            if self.config.doWrite:
                for (warpType, exposure) in exps.items():  # compatible w/ Py3
                    if exposure is not None:
                        self.log.info("Persisting %s" % self.getTempExpDatasetName(warpType))
                        tempExpRef.put(exposure, self.getTempExpDatasetName(warpType))
 
        return dataRefList
 
    @pipeBase.timeMethod
    def run(self, calExpList, ccdIdList, skyInfo, visitId=0, dataIdList=None):
        """Create a Warp from inputs
 
        We iterate over the multiple calexps in a single exposure to construct
        the warp (previously called a coaddTempExp) of that exposure to the
        supplied tract/patch.
 
        Pixels that receive no pixels are set to NAN; this is not correct
        (violates LSST algorithms group policy), but will be fixed up by
        interpolating after the coaddition.
 
        @param calexpRefList: List of data references for calexps that (may)
            overlap the patch of interest
        @param skyInfo: Struct from CoaddBaseTask.getSkyInfo() with geometric
            information about the patch
        @param visitId: integer identifier for visit, for the table that will
            produce the CoaddPsf
        @return a pipeBase Struct containing:
          - exposures: a dictionary containing the warps requested:
                "direct": direct warp if config.makeDirect
                "psfMatched": PSF-matched warp if config.makePsfMatched
        """
        warpTypeList = self.getWarpTypeList()
 
        totGoodPix = {warpType: 0 for warpType in warpTypeList}
        didSetMetadata = {warpType: False for warpType in warpTypeList}
        coaddTempExps = {warpType: self._prepareEmptyExposure(skyInfo) for warpType in warpTypeList}
        inputRecorder = {warpType: self.inputRecorder.makeCoaddTempExpRecorder(visitId, len(calExpList))
                         for warpType in warpTypeList}
 
        modelPsf = self.config.modelPsf.apply() if self.config.makePsfMatched else None
        if dataIdList is None:
            dataIdList = ccdIdList
 
        for calExpInd, (calExp, ccdId, dataId) in enumerate(zip(calExpList, ccdIdList, dataIdList)):
            self.log.info("Processing calexp %d of %d for this Warp: id=%s",
                          calExpInd+1, len(calExpList), dataId)
 
            try:
                warpedAndMatched = self.warpAndPsfMatch.run(calExp, modelPsf=modelPsf,
                                                            wcs=skyInfo.wcs, maxBBox=skyInfo.bbox,
                                                            makeDirect=self.config.makeDirect,
                                                            makePsfMatched=self.config.makePsfMatched)
            except Exception as e:
                self.log.warn("WarpAndPsfMatch failed for calexp %s; skipping it: %s", dataId, e)
                continue
            try:
                numGoodPix = {warpType: 0 for warpType in warpTypeList}
                for warpType in warpTypeList:
                    exposure = warpedAndMatched.getDict()[warpType]
                    if exposure is None:
                        continue
                    coaddTempExp = coaddTempExps[warpType]
                    if didSetMetadata[warpType]:
                        mimg = exposure.getMaskedImage()
                        mimg *= (coaddTempExp.getPhotoCalib().getInstFluxAtZeroMagnitude()
                                 / exposure.getPhotoCalib().getInstFluxAtZeroMagnitude())
                        del mimg
                    numGoodPix[warpType] = coaddUtils.copyGoodPixels(
                        coaddTempExp.getMaskedImage(), exposure.getMaskedImage(), self.getBadPixelMask())
                    totGoodPix[warpType] += numGoodPix[warpType]
                    self.log.debug("Calexp %s has %d good pixels in this patch (%.1f%%) for %s",
                                   dataId, numGoodPix[warpType],
                                   100.0*numGoodPix[warpType]/skyInfo.bbox.getArea(), warpType)
                    if numGoodPix[warpType] > 0 and not didSetMetadata[warpType]:
                        coaddTempExp.setPhotoCalib(exposure.getPhotoCalib())
                        coaddTempExp.setFilter(exposure.getFilter())
                        coaddTempExp.getInfo().setVisitInfo(exposure.getInfo().getVisitInfo())
                        # PSF replaced with CoaddPsf after loop if and only if creating direct warp
                        coaddTempExp.setPsf(exposure.getPsf())
                        didSetMetadata[warpType] = True
 
                    # Need inputRecorder for CoaddApCorrMap for both direct and PSF-matched
                    inputRecorder[warpType].addCalExp(calExp, ccdId, numGoodPix[warpType])
 
            except Exception as e:
                self.log.warn("Error processing calexp %s; skipping it: %s", dataId, e)
                continue
 
        for warpType in warpTypeList:
            self.log.info("%sWarp has %d good pixels (%.1f%%)",
                          warpType, totGoodPix[warpType], 100.0*totGoodPix[warpType]/skyInfo.bbox.getArea())
 
            if totGoodPix[warpType] > 0 and didSetMetadata[warpType]:
                inputRecorder[warpType].finish(coaddTempExps[warpType], totGoodPix[warpType])
                if warpType == "direct":
                    coaddTempExps[warpType].setPsf(
                        CoaddPsf(inputRecorder[warpType].coaddInputs.ccds, skyInfo.wcs,
                                 self.config.coaddPsf.makeControl()))
            else:
                if not self.config.doWriteEmptyWarps:
                    # No good pixels. Exposure still empty
                    coaddTempExps[warpType] = None
 
        result = pipeBase.Struct(exposures=coaddTempExps)
        return result
 
    def getCalibratedExposure(self, dataRef, bgSubtracted):
        """Return one calibrated Exposure, possibly with an updated SkyWcs.
 
        @param[in] dataRef        a sensor-level data reference
        @param[in] bgSubtracted   return calexp with background subtracted? If False get the
                                  calexp's background background model and add it to the calexp.
        @return calibrated exposure
 
        @raises MissingExposureError If data for the exposure is not available.
 
        If config.doApplyExternalPhotoCalib is `True`, the photometric calibration
        (`photoCalib`) is taken from `config.externalPhotoCalibName` via the
        `name_photoCalib` dataset.  Otherwise, the photometric calibration is
        retrieved from the processed exposure.  When
        `config.doApplyExternalSkyWcs` is `True`, the astrometric calibration
        is taken from `config.externalSkyWcsName` with the `name_wcs` dataset.
        Otherwise, the astrometric calibration is taken from the processed
        exposure.
        """
        try:
            exposure = dataRef.get(self.calexpType, immediate=True)
        except dafPersist.NoResults as e:
            raise MissingExposureError('Exposure not found: %s ' % str(e)) from e
 
        if not bgSubtracted:
            background = dataRef.get("calexpBackground", immediate=True)
            mi = exposure.getMaskedImage()
            mi += background.getImage()
            del mi
 
        if self.config.doApplyExternalPhotoCalib:
            source = f"{self.config.externalPhotoCalibName}_photoCalib"
            self.log.debug("Applying external photoCalib to %s from %s", dataRef.dataId, source)
            photoCalib = dataRef.get(source)
            exposure.setPhotoCalib(photoCalib)
        else:
            photoCalib = exposure.getPhotoCalib()
 
        if self.config.doApplyExternalSkyWcs:
            source = f"{self.config.externalSkyWcsName}_wcs"
            self.log.debug("Applying external skyWcs to %s from %s", dataRef.dataId, source)
            skyWcs = dataRef.get(source)
            exposure.setWcs(skyWcs)
 
        exposure.maskedImage = photoCalib.calibrateImage(exposure.maskedImage,
                                                         includeScaleUncertainty=self.config.includeCalibVar)
        exposure.maskedImage /= photoCalib.getCalibrationMean()
        # TODO: The images will have a calibration of 1.0 everywhere once RFC-545 is implemented.
        # exposure.setCalib(afwImage.Calib(1.0))
        return exposure
 
    @staticmethod
    def _prepareEmptyExposure(skyInfo):
        """Produce an empty exposure for a given patch"""
        exp = afwImage.ExposureF(skyInfo.bbox, skyInfo.wcs)
        exp.getMaskedImage().set(numpy.nan, afwImage.Mask
                                 .getPlaneBitMask("NO_DATA"), numpy.inf)
        return exp
 
    def getWarpTypeList(self):
        """Return list of requested warp types per the config.
        """
        warpTypeList = []
        if self.config.makeDirect:
            warpTypeList.append("direct")
        if self.config.makePsfMatched:
            warpTypeList.append("psfMatched")
        return warpTypeList
 
    def applySkyCorr(self, dataRef, calexp):
        """Apply correction to the sky background level
 
        Sky corrections can be generated with the 'skyCorrection.py'
        executable in pipe_drivers. Because the sky model used by that
        code extends over the entire focal plane, this can produce
        better sky subtraction.
 
        The calexp is updated in-place.
 
        Parameters
        ----------
        dataRef : `lsst.daf.persistence.ButlerDataRef`
            Data reference for calexp.
        calexp : `lsst.afw.image.Exposure` or `lsst.afw.image.MaskedImage`
            Calibrated exposure.
        """
        bg = dataRef.get("skyCorr")
        self.log.debug("Applying sky correction to %s", dataRef.dataId)
        if isinstance(calexp, afwImage.Exposure):
            calexp = calexp.getMaskedImage()
        calexp -= bg.getImage()
 
 
class MakeWarpConnections(pipeBase.PipelineTaskConnections,
                          dimensions=("tract", "patch", "skymap", "instrument", "visit"),
                          defaultTemplates={"coaddName": "deep"}):
    calExpList = cT.Input(
        doc="Input exposures to be resampled and optionally PSF-matched onto a SkyMap projection/patch",
        name="calexp",
        storageClass="ExposureF",
        dimensions=("instrument", "visit", "detector"),
        multiple=True,
    )
    backgroundList = cT.Input(
        doc="Input backgrounds to be added back into the calexp if bgSubtracted=False",
        name="calexpBackground",
        storageClass="Background",
        dimensions=("instrument", "visit", "detector"),
        multiple=True,
    )
    skyCorrList = cT.Input(
        doc="Input Sky Correction to be subtracted from the calexp if doApplySkyCorr=True",
        name="skyCorr",
        storageClass="Background",
        dimensions=("instrument", "visit", "detector"),
        multiple=True,
    )
    skyMap = cT.Input(
        doc="Input definition of geometry/bbox and projection/wcs for warped exposures",
        name="{coaddName}Coadd_skyMap",
        storageClass="SkyMap",
        dimensions=("skymap",),
    )
    direct = cT.Output(
        doc=("Output direct warped exposure (previously called CoaddTempExp), produced by resampling ",
             "calexps onto the skyMap patch geometry."),
        name="{coaddName}Coadd_directWarp",
        storageClass="ExposureF",
        dimensions=("tract", "patch", "skymap", "visit", "instrument"),
    )
    psfMatched = cT.Output(
        doc=("Output PSF-Matched warped exposure (previously called CoaddTempExp), produced by resampling ",
             "calexps onto the skyMap patch geometry and PSF-matching to a model PSF."),
        name="{coaddName}Coadd_psfMatchedWarp",
        storageClass="ExposureF",
        dimensions=("tract", "patch", "skymap", "visit", "instrument"),
    )
 
    def __init__(self, *, config=None):
        super().__init__(config=config)
        if config.bgSubtracted:
            self.inputs.remove("backgroundList")
        if not config.doApplySkyCorr:
            self.inputs.remove("skyCorrList")
        if not config.makeDirect:
            self.outputs.remove("direct")
        if not config.makePsfMatched:
            self.outputs.remove("psfMatched")
 
 
class MakeWarpConfig(pipeBase.PipelineTaskConfig, MakeCoaddTempExpConfig,
                     pipelineConnections=MakeWarpConnections):
 
    def validate(self):
        super().validate()
        # TODO: Remove this constraint after DM-17062
        if self.doApplyExternalPhotoCalib:
            raise RuntimeError("Gen3 MakeWarpTask cannot apply external PhotoCalib results. "
                               "Please set doApplyExternalPhotoCalib=False.")
        if self.doApplyExternalSkyWcs:
            raise RuntimeError("Gen3 MakeWarpTask cannot apply external SkyWcs results. "
                               "Please set doApplyExternalSkyWcs=False.")
 
 
class MakeWarpTask(MakeCoaddTempExpTask, pipeBase.PipelineTask):
    """Warp and optionally PSF-Match calexps onto an a common projection
 
    First Draft of a Gen3 compatible MakeWarpTask which
    currently does not handle doApplyExternalPhotoCalib=True or
    doApplyExternalSkyWcs=True.
    """
    ConfigClass = MakeWarpConfig
    _DefaultName = "makeWarp"
 
    @utils.inheritDoc(pipeBase.PipelineTask)
    def runQuantum(self, butlerQC, inputRefs, outputRefs):
        """
        Notes
        ----
        Construct warps for requested warp type for single epoch
 
        PipelineTask (Gen3) entry point to warp and optionally PSF-match
        calexps. This method is analogous to `runDataRef`.
        """
        # Read in all inputs.
        inputs = butlerQC.get(inputRefs)
 
        # Construct skyInfo expected by `run`.  We remove the SkyMap itself
        # from the dictionary so we can pass it as kwargs later.
        skyMap = inputs.pop("skyMap")
        quantumDataId = butlerQC.quantum.dataId
        skyInfo = makeSkyInfo(skyMap, tractId=quantumDataId['tract'], patchId=quantumDataId['patch'])
 
        # Construct list of input DataIds expected by `run`
        dataIdList = [ref.dataId for ref in inputRefs.calExpList]
 
        # Construct list of packed integer IDs expected by `run`
        ccdIdList = [dataId.pack("visit_detector") for dataId in dataIdList]
 
        # Extract integer visitId requested by `run`
        visits = [dataId['visit'] for dataId in dataIdList]
        assert(all(visits[0] == visit for visit in visits))
        visitId = visits[0]
 
        self.prepareCalibratedExposures(**inputs)
        results = self.run(**inputs, visitId=visitId, ccdIdList=ccdIdList, dataIdList=dataIdList,
                           skyInfo=skyInfo)
        if self.config.makeDirect:
            butlerQC.put(results.exposures["direct"], outputRefs.direct)
        if self.config.makePsfMatched:
            butlerQC.put(results.exposures["psfMatched"], outputRefs.psfMatched)
 
    def prepareCalibratedExposures(self, calExpList, backgroundList=None, skyCorrList=None):
        """Calibrate and add backgrounds to input calExpList in place
 
        TODO DM-17062: apply jointcal/meas_mosaic here
 
        Parameters
        ----------
        calExpList : `list` of `lsst.afw.image.Exposure`
            Sequence of calexps to be modified in place
        backgroundList : `list` of `lsst.afw.math.backgroundList`
            Sequence of backgrounds to be added back in if bgSubtracted=False
        skyCorrList : `list` of `lsst.afw.math.backgroundList`
            Sequence of background corrections to be subtracted if doApplySkyCorr=True
        """
        backgroundList = len(calExpList)*[None] if backgroundList is None else backgroundList
        skyCorrList = len(calExpList)*[None] if skyCorrList is None else skyCorrList
        for calexp, background, skyCorr in zip(calExpList, backgroundList, skyCorrList):
            mi = calexp.maskedImage
            if not self.config.bgSubtracted:
                mi += background.getImage()
            if self.config.doApplySkyCorr:
                mi -= skyCorr.getImage()