sfm.py

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#!/usr/bin/env python
#
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"""Base classes for single-frame measurement plugins and the driver task for these.

In single-frame measurement, we assume that detection and probably deblending have already been run on
the same frame, so a SourceCatalog has already been created with Footprints (which may be HeavyFootprints).
Measurements are generally recorded in the coordinate system of the image being measured (and all
slot-eligible fields must be), but non-slot fields may be recorded in other coordinate systems if necessary
to avoid information loss (this should, of course, be indicated in the field documentation).
"""

from .pluginRegistry import PluginRegistry
from .baseMeasurement import BasePluginConfig, BasePlugin, BaseMeasurementConfig, BaseMeasurementTask
from .noiseReplacer import NoiseReplacer, DummyNoiseReplacer

__all__ = ("SingleFramePluginConfig", "SingleFramePlugin",
           "SingleFrameMeasurementConfig", "SingleFrameMeasurementTask")

class SingleFramePluginConfig(BasePluginConfig):
    """!
    Base class for configs of single-frame plugin algorithms.
    """
    pass

class SingleFramePlugin(BasePlugin):
    """!
    Base class for single-frame plugin algorithms.

    New Plugins can be created in Python by inheriting directly from this class
    and implementing measure(), fail() (from BasePlugin), and optionally __init__
    and measureN().  Plugins can also be defined in C++ via the WrappedSingleFramePlugin
    class.
    """

    # All subclasses of SingleFramePlugin should be registered here
    registry = PluginRegistry(SingleFramePluginConfig)
    ConfigClass = SingleFramePluginConfig

    def __init__(self, config, name, schema, metadata):
        """!
        Initialize the measurement object.

        @param[in]  config       An instance of this class's ConfigClass.
        @param[in]  name         The string the plugin was registered with.
        @param[in,out]  schema   The Source schema.  New fields should be added here to
                                 hold measurements produced by this plugin.
        @param[in]  metadata     Plugin metadata that will be attached to the output catalog
        """
        BasePlugin.__init__(self, config, name)

    def measure(self, measRecord, exposure):
        """!
        Measure the properties of a source on a single image (single-epoch image or coadd).

        @param[in,out] measRecord  lsst.afw.table.SourceRecord to be filled with outputs,
                                   and from which previously-measured quantities can be
                                   retreived.

        @param[in] exposure      lsst.afw.image.ExposureF, containing the pixel data to
                                 be measured and the associated Psf, Wcs, etc.  All
                                 other sources in the image will have been replaced by
                                 noise according to deblender outputs.

        """
        raise NotImplementedError()

    def measureN(self, measCat, exposure):
        """!
        Measure the properties of a group of blended sources on a single image
        (single-epoch image or coadd).

        @param[in,out] measCat   lsst.afw.table.SourceCatalog to be filled with outputs,
                                 and from which previously-measured quantities can be
                                 retrieved, containing only the sources that should be
                                 measured together in this call.

        @param[in] exposure      lsst.afw.image.ExposureF, containing the pixel data to
                                 be measured and the associated Psf, Wcs, etc.  Sources
                                 not in the blended hierarchy to be measured will have
                                 been replaced with noise using deblender outputs.

        Derived classes that do not implement measureN() should just inherit this
        disabled version.  Derived classes that do implement measureN() should additionally
        add a bool doMeasureN config field to their config class to signal that measureN-mode
        is available.
        """
        raise NotImplementedError()

class SingleFrameMeasurementConfig(BaseMeasurementConfig):
    """!
    Config class for single frame measurement driver task.
    """

    plugins = SingleFramePlugin.registry.makeField(
        multi=True,
        default=["base_PixelFlags",
                 "base_SdssCentroid",
                 "base_GaussianCentroid",
                 "base_NaiveCentroid",
                 "base_SdssShape",
                 "base_GaussianFlux",
                 "base_PsfFlux",
                 "base_CircularApertureFlux",
                 "base_ClassificationExtendedness",
                 "base_SkyCoord",
                 ],
        doc="Plugins to be run and their configuration"
        )
    algorithms = property(lambda self: self.plugins, doc="backwards-compatibility alias for plugins")

## \addtogroup LSST_task_documentation
## \{
## \page SingleFrameMeasurementTask
## \ref SingleFrameMeasurementTask_ "SingleFrameMeasurementTask"
## \copybrief SingleFrameMeasurementTask
## \}

class SingleFrameMeasurementTask(BaseMeasurementTask):
    """!
    \anchor SingleFrameMeasurementTask_

    \brief A subtask for measuring the properties of sources on a single exposure.

    The task is configured with a list of "plugins": each plugin defines the values it
    measures (i.e. the columns in a table it will fill) and conducts that measurement
    on each detected source (see SingleFramePlugin).  The job of the
    measurement task is to initialize the set of plugins (which includes setting up the
    catalog schema) from their configuration, and then invoke each plugin on each
    source.

    When run after the deblender (see lsst.meas.deblender.SourceDeblendTask),
    SingleFrameMeasurementTask also replaces each source's neighbors with noise before
    measuring each source, utilizing the HeavyFootprints created by the deblender (see
    NoiseReplacer).

    SingleFrameMeasurementTask has only two methods: __init__() and run().  For configuration
    options, see SingleFrameMeasurementConfig.

    @section meas_base_sfm_Example      A complete example of using SingleFrameMeasurementTask

    The code below is in examples/runSingleFrameTask.py

    @dontinclude runSingleFrameTask.py

    See meas_algorithms_detection_Example for more information on SourceDetectionTask.

    First, import the required tasks (there are some other standard imports;
    read the file if you're confused):

    @skip SourceDetectionTask
    @until SingleFrameMeasurementTask

    We need to create our tasks before processing any data as the task constructors
    can add extra columns to the schema.  The most important argument we pass these to these
    is an lsst.afw.table.Schema object, which contains information about the fields (i.e. columns) of the
    measurement catalog we'll create, including names, types, and additional documentation.
    Tasks that operate on a catalog are typically passed a Schema upon construction, to which
    they add the fields they'll fill later when run.  We construct a mostly empty Schema that
    contains just the fields required for a SourceCatalog like this:

    @skipline schema

    Now we can configure and create the SourceDetectionTask:

    @until detectionTask

    We then move on to configuring the measurement task:

    @until config

    While a reasonable set of plugins is configured by default, we'll customize the list.
    We also need to unset one of the slots at the same time, because we're
    not running the algorithm that it's set to by default, and that would cause problems later:

    @until psfFlux

    Now, finally, we can construct the measurement task:

    @skipline measureTask

    After constructing all the tasks, we can inspect the Schema we've created:

    @skipline print schema

    All of the fields in the
    schema can be accessed via the get() method on a record object.  See afwTable for more
    information.

    We're now ready to process the data (we could loop over multiple exposures/catalogs using the same
    task objects).  First create the output table and process the image to find sources:

    @skipline afwTable
    @skip result
    @until sources

    Then measure them:

    @skipline measure

    We then might plot the results (@em e.g. if you set `--ds9` on the command line)

    @skip display
    @until RED

    and end up with something like

    @image html runSingleFrameTask-ds9.png
    """

    ConfigClass = SingleFrameMeasurementConfig

    def __init__(self, schema, algMetadata=None, **kwds):
        """!
        Initialize the task. Set up the execution order of the plugins and initialize
        the plugins, giving each plugin an opportunity to add its measurement fields to
        the output schema and to record information in the task metadata.

        @param[in,out] schema      lsst.afw.table.Schema, to be initialized to include the
                                   measurement fields from the plugins already
        @param[in,out] algMetadata lsst.daf.base.PropertyList used to record information about
                                   each algorithm.  An empty PropertyList will be created if None.
        @param[in]     **kwds      Keyword arguments forwarded to lsst.pipe.base.Task.__init__
        """
        super(SingleFrameMeasurementTask, self).__init__(algMetadata=algMetadata, **kwds)
        self.schema = schema
        self.config.slots.setupSchema(self.schema)
        self.initializePlugins(schema=self.schema)
        self.makeSubtask("applyApCorr", schema=self.schema)

    def run(self, measCat, exposure, noiseImage=None, exposureId=None, beginOrder=None, endOrder=None,
        allowApCorr=True):
        """!
        Run single frame measurement over an exposure and source catalog

        @param[in,out]  measCat  lsst.afw.table.SourceCatalog to be filled with outputs.  Must
                                 contain all the SourceRecords to be measured (with Footprints
                                 attached), and have a schema that is a superset of self.schema.

        @param[in] exposure      lsst.afw.image.ExposureF, containing the pixel data to
                                 be measured and the associated Psf, Wcs, etc.
        @param[in] noiseImage    optional lsst.afw.image.ImageF for test which need to control
                                 noiseReplacement
        @param[in] exposureId    optional unique exposureId used to calculate random number
                                 generator seed in the NoiseReplacer.
        @param[in] beginOrder    beginning execution order (inclusive): measurements with
                                 executionOrder < beginOrder are not executed. None for no limit.
        @param[in] endOrder      ending execution order (exclusive): measurements with
                                 executionOrder >= endOrder are not executed. None for no limit.
        @param[in] allowApCorr  allow application of aperture correction?
        """
        # Temporary workaround for change in order of arguments; will be removed when transition
        # from meas_algorithms to meas_base is complete.
        if exposure.__class__.__name__ == "SourceCatalog":
            temp = exposure
            exposure = measCat
            measCat = temp
        assert measCat.getSchema().contains(self.schema)
        footprints = {measRecord.getId(): (measRecord.getParent(), measRecord.getFootprint())
            for measRecord in measCat}

        # noiseReplacer is used to fill the footprints with noise and save heavy footprints
        # of the source pixels so that they can be restored one at a time for measurement.
        # After the NoiseReplacer is constructed, all pixels in the exposure.getMaskedImage()
        # which belong to objects in measCat will be replaced with noise
        if self.config.doReplaceWithNoise:
            noiseReplacer = NoiseReplacer(self.config.noiseReplacer, exposure, footprints,
                                          noiseImage=noiseImage, log=self.log, exposureId=exposureId)
            algMetadata = measCat.getMetadata()
            if not algMetadata is None:
                algMetadata.addInt("NOISE_SEED_MULTIPLIER", self.config.noiseReplacer.noiseSeedMultiplier)
                algMetadata.addString("NOISE_SOURCE", self.config.noiseReplacer.noiseSource)
                algMetadata.addDouble("NOISE_OFFSET", self.config.noiseReplacer.noiseOffset)
                if not exposureId is None:
                    algMetadata.addLong("NOISE_EXPOSURE_ID", exposureId)
        else:
            noiseReplacer = DummyNoiseReplacer()

        # First, create a catalog of all parentless sources
        # Loop through all the parent sources, first processing the children, then the parent
        measParentCat = measCat.getChildren(0)

        self.log.info("Measuring %d sources (%d parents, %d children) "
                      % (len(measCat), len(measParentCat), len(measCat) - len(measParentCat)))

        for parentIdx, measParentRecord in enumerate(measParentCat):
            # first get all the children of this parent, insert footprint in turn, and measure
            measChildCat = measCat.getChildren(measParentRecord.getId())
            # TODO: skip this loop if there are no plugins configured for single-object mode
            for measChildRecord in measChildCat:
                noiseReplacer.insertSource(measChildRecord.getId())
                self.callMeasure(measChildRecord, exposure, beginOrder=beginOrder, endOrder=endOrder)
                noiseReplacer.removeSource(measChildRecord.getId())
            # Then insert the parent footprint, and measure that
            noiseReplacer.insertSource(measParentRecord.getId())
            self.callMeasure(measParentRecord, exposure, beginOrder=beginOrder, endOrder=endOrder)
            # Finally, process both the parent and the child set through measureN
            self.callMeasureN(measParentCat[parentIdx:parentIdx+1], exposure,
                    beginOrder=beginOrder, endOrder=endOrder)
            self.callMeasureN(measChildCat, exposure, beginOrder=beginOrder, endOrder=endOrder)
            noiseReplacer.removeSource(measParentRecord.getId())
        # when done, restore the exposure to its original state
        noiseReplacer.end()

        if allowApCorr:
            self._applyApCorrIfWanted(
                sources = measCat,
                apCorrMap = exposure.getInfo().getApCorrMap(),
                endOrder = endOrder,
            )

    def measure(self, measCat, exposure):
        """!
        Backwards-compatibility alias for run()
        """
        self.run(measCat, exposure)