quickFrameMeasurement.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
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import numpy as np
import lsst.afw.detection as afwDetect
import lsst.afw.table as afwTable
import lsst.meas.base as measBase
import lsst.daf.base as dafBase
import lsst.pipe.base as pipeBase
import lsst.pex.config as pexConfig
from lsst.meas.base import MeasurementError
from lsst.meas.algorithms.installGaussianPsf import InstallGaussianPsfTask
 
 
class QuickFrameMeasurementTaskConfig(pexConfig.Config):
    """Config class for the QuickFrameMeasurementTask.
    """
    installPsf = pexConfig.ConfigurableField(
        target=InstallGaussianPsfTask,
        doc="Task for installing an initial PSF",
    )
    maxNonRoundness = pexConfig.Field(
        dtype=float,
        doc="Ratio of xx to yy (or vice versa) above which to cut, in order to exclude spectra",
        default=5.,
    )
    maxExtendedness = pexConfig.Field(
        dtype=float,
        doc="Max absolute value of xx and yy above which to cut, in order to exclude large/things",
        default=100,
    )
    doExtendednessCut = pexConfig.Field(
        dtype=bool,
        doc="Apply the extendeness cut, as definted by maxExtendedness",
        default=False,
    )
    centroidPixelPercentile = pexConfig.Field(
        dtype=float,
        doc="The image's percentile value which the centroid must be greater than to pass the final peak"
            " check. Ignored if doCheckCentroidPixelValue is False",
        default=90,
    )
    doCheckCentroidPixelValue = pexConfig.Field(
        dtype=bool,
        doc="Check that the centroid found is actually in the centroidPixelPercentile percentile of the"
            " image? Set to False for donut images.",
        default=True,
    )
    initialPsfWidth = pexConfig.Field(
        dtype=float,
        doc="Guess at the initial PSF FWHM in pixels.",
        default=10,
    )
    nSigmaDetection = pexConfig.Field(
        dtype=float,
        doc="Number of sigma for the detection limit.",
        default=20,
    )
    nPixMinDetection = pexConfig.Field(
        dtype=int,
        doc="Minimum number of pixels in a detected source.",
        default=10,
    )
 
    def setDefaults(self):
        super().setDefaults()
        self.installPsfinstallPsf.fwhm = self.initialPsfWidthinitialPsfWidth
 
 
class QuickFrameMeasurementTask(pipeBase.Task):
    """WARNING: An experimental new task with changable API! Do not rely on yet!
 
    This task finds the centroid of the brightest source in a given CCD-image
    and returns its centroid and a rough estimate of the seeing/PSF.
 
    It is designed for speed, such that it can be used in observing scripts
    to provide pointing offsets, allowing subsequent pointings to place
    a source at an exact pixel position.
 
    The approach taken here is deliberately sub-optimal in the detection and
    measurement sense, with all optimisation being done for speed and robustness
    of the result.
 
    A small set of unit tests exist for this task, which run automatically
    if afwdata is setup. These, however, are stricky unit tests, and will not
    catch algorithmic regressions. TODO: DM-29038 exists to merge a regression
    real test which runs against 1,000 LATISS images, but is therefore slow
    and requires access to the data.
 
    Parameters
    ----------
    config : lsst.pipe.tasks.quickFrameMeasurement.QuickFrameMeasurementTaskConfig
        Configuration class for the QuickFrameMeasurementTask.
 
    display : lsst.afw.display.Display, optional
        The display to use for showing the images, detections and centroids.
 
    Returns
    -------
    result : lsst.pipe.base.Struct()
        Return strucure containing whether the task was successful, the main
        source's centroid, its the aperture fluxes, the ixx and iyy of the
        source, and the median ixx, iyy of the detections in the exposure.
        See run() method for further details.
 
    Raises
    ------
    This task should *never* raise, as the run() method is enclosed in an
    except Exception block, so that it will never fail during observing.
    Failure modes should be limited to returning a return Struct() with the same
    structure as the success case, with all value set to np.nan but with
    result.success=False.
    """
    ConfigClass = QuickFrameMeasurementTaskConfig
    _DefaultName = 'quickFrameMeasurementTask'
 
    def __init__(self, config, *, display=None, **kwargs):
        super().__init__(config=config, **kwargs)
        self.makeSubtask("installPsf")
 
        self.displaydisplay = None
        if display:
            self.displaydisplay = display
 
        self.centroidNamecentroidName = "base_SdssCentroid"
        self.shapeNameshapeName = "base_SdssShape"
        self.schemaschema = afwTable.SourceTable.makeMinimalSchema()
        self.schemaschema.getAliasMap().set("slot_Centroid", self.centroidNamecentroidName)
        self.schemaschema.getAliasMap().set("slot_Shape", self.shapeNameshapeName)
        self.controlcontrol = measBase.SdssCentroidControl()
        self.centroidercentroider = measBase.SdssCentroidAlgorithm(self.controlcontrol, self.centroidNamecentroidName, self.schemaschema)
        self.sdssShapesdssShape = measBase.SdssShapeControl()
        self.shapershaper = measBase.SdssShapeAlgorithm(self.sdssShapesdssShape, self.shapeNameshapeName, self.schemaschema)
        self.apFluxControlapFluxControl = measBase.ApertureFluxControl()
        md = dafBase.PropertySet()
        self.apFluxerapFluxer = measBase.CircularApertureFluxAlgorithm(self.apFluxControlapFluxControl, "aperFlux",
                                                               self.schemaschema, md)
 
        self.tabletable = afwTable.SourceTable.make(self.schemaschema)  # make sure to call this last!
 
    @staticmethod
    def detectObjectsInExp(exp, nSigma, nPixMin, grow=0):
        """Run a very basic but fast threshold-based object detection on an exposure
        Return the footPrintSet for the objects in a postISR exposure.
 
        Parameters
        ----------
        exp : lsst.afw.image.Exposure
            Image in which to detect objects.
 
        nSigma : float
            nSigma above image's stddev at which to set the detection threshold.
 
        nPixMin : int
            Minimum number of pixels for detection.
 
        grow : int
            Grow the detected footprint by this many pixels.
 
        Returns
        -------
        footPrintSet : lsst.afw.detection.FootprintSet
            FootprintSet containing the detections.
        """
        threshold = afwDetect.Threshold(nSigma, afwDetect.Threshold.STDEV)
        footPrintSet = afwDetect.FootprintSet(exp.getMaskedImage(), threshold, "DETECTED", nPixMin)
        if grow > 0:
            isotropic = True
            footPrintSet = afwDetect.FootprintSet(footPrintSet, grow, isotropic)
        return footPrintSet
 
    @staticmethod
    def checkResult(exp, centroid, srcNum, percentile):
        """Perform a final check that centroid location is actually bright.
 
        Parameters
        ----------
        exp : lsst.afw.image.Exposure
        centroid : `tuple` of `float`
            Location of the centroid in pixel coordinates
 
        scrNum : int
            Number of the source in the source catalog. Only used if the check
            is failed, for debug purposes.
 
        percentile : float
            Image's percentile above which the pixel containing the centroid
            must be in order to pass the check.
 
        Raises
        ------
        ValueError
            Raised if the centroid's pixel is not above the percentile threshold
        """
        threshold = np.percentile(exp.image.array, percentile)
        pixelValue = exp.image[centroid]
        if pixelValue < threshold:
            msg = (f"Final centroid pixel value check failed: srcNum {srcNum} at {centroid}"
                   f" has central pixel = {pixelValue:3f} <"
                   f" {percentile} percentile of image = {threshold:3f}")
            raise ValueError(msg)
        return
 
    @staticmethod
    def _calcMedianXxYy(objData):
        """Return the median ixx and iyy for object in the image.
        """
        medianXx = np.nanmedian([element['xx'] for element in objData.values()])
        medianYy = np.nanmedian([element['xx'] for element in objData.values()])
        return medianXx, medianYy
 
    def _calcBrightestObjSrcNum(self, objData):
        """Find the brightest source which passes the cuts among the sources.
 
        Parameters
        ----------
        objData : `dict` of `dict`
            Dictionary, keyed by source number, containing the measurements.
 
        Returns
        -------
        srcNum : int
            The source number of the brightest source which passes the cuts.
        """
        max70, max70srcNum = -1, -1
        max25, max25srcNum = -1, -1
 
        for srcNum in sorted(objData.keys()):  # srcNum not contiguous so don't use a list comp
            # skip flag used rather than continue statements so we have all the
            # metrics computed for debug purposes as this task is whack-a-mole
            skip = False
            xx = objData[srcNum]['xx']
            yy = objData[srcNum]['yy']
 
            xx = max(xx, 1e-9)  # need to protect against division by zero
            yy = max(yy, 1e-9)  # because we don't `continue` on zero moments
 
            if self.config.doExtendednessCut:
                if xx > self.config.maxExtendedness or yy > self.config.maxExtendedness:
                    skip = True
 
            nonRoundness = xx/yy
            nonRoundness = max(nonRoundness, 1/nonRoundness)
            if nonRoundness > self.config.maxNonRoundness:
                skip = True
 
            if self.log.isDebugEnabled():
                text = f"src {srcNum}: {objData[srcNum]['xCentroid']:.0f}, {objData[srcNum]['yCentroid']:.0f}"
                text += f" - xx={xx:.1f}, yy={yy:.1f}, nonRound={nonRoundness:.1f}"
                text += f" - ap70={objData[srcNum]['apFlux70']:,.0f}"
                text += f" - ap25={objData[srcNum]['apFlux25']:,.0f}"
                text += f" - skip={skip}"
                self.log.debug(text)
 
            if skip:
                continue
 
            ap70 = objData[srcNum]['apFlux70']
            ap25 = objData[srcNum]['apFlux25']
            if ap70 > max70:
                max70 = ap70
                max70srcNum = srcNum
            if ap25 > max25:
                max25 = ap25
                max25srcNum = srcNum
        if max70srcNum != max25srcNum:
            self.log.warn("WARNING! Max apFlux70 for different object than with max apFlux25")
 
        if max70srcNum >= 0:  # starts as -1, return None if nothing is acceptable
            return max70srcNum
        return None
 
    def _measureFp(self, fp, exp):
        """Run the measurements on a footprint.
 
        Parameters
        ----------
        fp : lsst.afw.detection.Footprint
            The footprint to measure.
 
        exp : lsst.afw.image.Exposure
            The footprint's parent exposure.
 
        Returns
        -------
        src : lsst.afw.table.SourceRecord
            The source record containing the measurements.
        """
        src = self.tabletable.makeRecord()
        src.setFootprint(fp)
        self.centroidercentroider.measure(src, exp)
        self.shapershaper.measure(src, exp)
        self.apFluxerapFluxer.measure(src, exp)
        return src
 
    def _getDataFromSrcRecord(self, src):
        """Extract the shapes and centroids from a source record.
 
        Parameters
        ----------
        src : lsst.afw.table.SourceRecord
            The source record from which to extract the measurements.
 
        Returns
        -------
        srcData : lsst.pipe.base.Struct
            The struct containing the extracted measurements.
        """
        pScale = self.plateScaleplateScale
        xx = np.sqrt(src['base_SdssShape_xx'])*2.355*pScale  # 2.355 for FWHM, pScale for platescale from exp
        yy = np.sqrt(src['base_SdssShape_yy'])*2.355*pScale
        xCentroid = src['base_SdssCentroid_x']
        yCentroid = src['base_SdssCentroid_y']
        # apFluxes available: 70, 50, 35, 25, 17, 12 9, 6, 4.5, 3
        apFlux70 = src['aperFlux_70_0_instFlux']
        apFlux25 = src['aperFlux_25_0_instFlux']
        return pipeBase.Struct(xx=xx,
                               yy=yy,
                               xCentroid=xCentroid,
                               yCentroid=yCentroid,
                               apFlux70=apFlux70,
                               apFlux25=apFlux25)
 
    @staticmethod
    def _getDataFromFootprintOnly(fp, exp):
        """Get the shape, centroid and flux from a footprint.
 
        Parameters
        ----------
        fp : lsst.afw.detection.Footprint
            The footprint to measure.
        exp : lsst.afw.image.Exposure
            The footprint's parent exposure.
 
        Returns
        -------
        srcData : lsst.pipe.base.Struct
            The struct containing the extracted measurements.
        """
        xx = fp.getShape().getIxx()
        yy = fp.getShape().getIyy()
        xCentroid, yCentroid = fp.getCentroid()
        apFlux70 = np.sum(exp[fp.getBBox()].image.array)
        apFlux25 = np.sum(exp[fp.getBBox()].image.array)
        return pipeBase.Struct(xx=xx,
                               yy=yy,
                               xCentroid=xCentroid,
                               yCentroid=yCentroid,
                               apFlux70=apFlux70,
                               apFlux25=apFlux25)
 
    @staticmethod
    def _measurementResultToDict(measurementResult):
        """Convenience function to repackage measurement results to a dict.
 
        Parameters
        ----------
        measurementResult : lsst.afw.table.SourceRecord
            The source record to convert to a dict.
 
        Returns
        -------
        objData : `dict`
            The dict containing the extracted data.
        """
        objData = {}
        objData['xx'] = measurementResult.xx
        objData['yy'] = measurementResult.yy
        objData['xCentroid'] = measurementResult.xCentroid
        objData['yCentroid'] = measurementResult.yCentroid
        objData['apFlux70'] = measurementResult.apFlux70
        objData['apFlux25'] = measurementResult.apFlux25
        return objData
 
    @staticmethod
    def _makeEmptyReturnStruct():
        """Make the default/template return struct, with defaults to False/nan.
 
        Returns
        -------
        objData : lsst.pipe.base.Struct
            The default template return structure.
        """
        result = pipeBase.Struct()
        result.success = False
        result.brightestObjCentroid = (np.nan, np.nan)
        result.brightestObj_xXyY = (np.nan, np.nan)
        result.brightestObjApFlux70 = np.nan
        result.brightestObjApFlux25 = np.nan
        result.medianXxYy = (np.nan, np.nan)
        return result
 
    def run(self, exp, doDisplay=False):
        """Calculate position, flux and shape of the brightest star in an image.
 
        Given an an assembled (and at least minimally ISRed exposure),
        quickly and robustly calculate the centroid of the
        brightest star in the image.
 
        Parameters
        ----------
        exp : lsst.afw.image.Exposure
            The exposure in which to find and measure the brightest star.
 
        doDisplay : bool
            Display the image and found sources. A diplay object must have
            been passed to the task constructor.
 
        Returns
        -------
        result : lsst.pipe.base.Struct
            Struct containing:
                Whether the task ran successfully and found the object (bool)
                The object's centroid (float, float)
                The object's ixx, iyy (float, float)
                The object's 70 pixel aperture flux (float)
                The object's 25 pixel aperture flux (float)
                The images's median ixx, iyy (float, float)
            If unsuccessful, the success field is False and all other results
            are np.nan of the expected shape.
 
        Notes
        -----
        Because of this task's involvement in observing scripts, the run method
        should *never* raise. Failure modes are noted by returning a Struct with
        the same structure as the success case, with all value set to np.nan and
        result.success=False.
        """
        try:
            result = self._run_run(exp=exp, doDisplay=doDisplay)
            return result
        except Exception as e:
            self.log.warn(f"Failed to find main source centroid {e}")
            result = self._makeEmptyReturnStruct_makeEmptyReturnStruct()
            return result
 
    def _run(self, exp, doDisplay=False):
        """The actual run method, called by run()
 
        Behaviour is documented in detail in the main run().
        """
        self.plateScaleplateScale = exp.getWcs().getPixelScale().asArcseconds()
        median = np.nanmedian(exp.image.array)
        exp.image -= median  # is put back later
        self.installPsf.run(exp)
        sources = self.detectObjectsInExpdetectObjectsInExp(exp, nSigma=self.config.nSigmaDetection,
                                          nPixMin=self.config.nPixMinDetection)
 
        if doDisplay:
            if self.displaydisplay is None:
                raise RuntimeError("Display failed as no display provided during init()")
            self.displaydisplay.mtv(exp)
 
        fpSet = sources.getFootprints()
        self.log.info(f"Found {len(fpSet)} sources in exposure")
 
        objData = {}
        nMeasured = 0
 
        for srcNum, fp in enumerate(fpSet):
            try:
                src = self._measureFp_measureFp(fp, exp)
                result = self._getDataFromSrcRecord_getDataFromSrcRecord(src)
            except MeasurementError:
                try:
                    # gets shape and centroid from footprint
                    result = self._getDataFromFootprintOnly_getDataFromFootprintOnly(fp, exp)
                except MeasurementError as e:
                    self.log.info(f"Skipped measuring source {srcNum}: {e}")
                    continue
            objData[srcNum] = self._measurementResultToDict_measurementResultToDict(result)
            nMeasured += 1
 
        self.log.info(f"Measured {nMeasured} of {len(fpSet)} sources in exposure")
 
        medianXxYy = self._calcMedianXxYy_calcMedianXxYy(objData)
 
        brightestObjSrcNum = self._calcBrightestObjSrcNum_calcBrightestObjSrcNum(objData)
        if brightestObjSrcNum is None:
            raise RuntimeError("No sources in image passed cuts")
 
        x = objData[brightestObjSrcNum]['xCentroid']
        y = objData[brightestObjSrcNum]['yCentroid']
        brightestObjCentroid = (x, y)
        xx = objData[brightestObjSrcNum]['xx']
        yy = objData[brightestObjSrcNum]['yy']
        brightestObjApFlux70 = objData[brightestObjSrcNum]['apFlux70']
        brightestObjApFlux25 = objData[brightestObjSrcNum]['apFlux25']
 
        exp.image += median  # put background back in
        if self.config.doCheckCentroidPixelValue:
            self.checkResultcheckResult(exp, brightestObjCentroid, brightestObjSrcNum,
                             self.config.centroidPixelPercentile)
 
        result = self._makeEmptyReturnStruct_makeEmptyReturnStruct()
        result.success = True
        result.brightestObjCentroid = brightestObjCentroid
        result.brightestObj_xXyY = (xx, yy)
        result.brightestObjApFlux70 = brightestObjApFlux70
        result.brightestObjApFlux25 = brightestObjApFlux25
        result.medianXxYy = medianXxYy
        return result