ForcedGaapFluxPlugin#
- class lsst.meas.extensions.gaap.ForcedGaapFluxPlugin(config, name, schemaMapper, metadata, logName=None)#
Bases:
BaseGaapFluxMixin,ForcedPluginGaussian Aperture and PSF (GAaP) photometry plugin in forced mode.
This is the GAaP plugin to run for consistent colors across the bandpasses.
Parameters#
- config
GaapFluxConfig Plugin configuration.
- name
str Plugin name, for registering.
- schemaMapper
lsst.afw.table.SchemaMapper A mapping from reference catalog fields to output catalog fields. Output fields will be added to the output schema. for the measurement output catalog. New fields will be added to hold measurements produced by this plugin.
- metadata
lsst.daf.base.PropertySet Plugin metadata that will be attached to the output catalog.
- logName
str, optional Name to use when logging errors. This will be provided by the measurement framework.
Methods Summary
Get the relative execution order of this plugin.
measure(measRecord, exposure, refRecord, refWcs)Measure the properties of a source given an image and a reference.
Methods Documentation
- classmethod getExecutionOrder() float#
Get the relative execution order of this plugin.
Must be reimplemented as a class method by concrete derived classes.
- measure(measRecord, exposure, refRecord, refWcs)#
Measure the properties of a source given an image and a reference.
Parameters#
- exposure
lsst.afw.image.ExposureF The pixel data to be measured, together with the associated PSF, WCS, etc. All other sources in the image should have been replaced by noise according to deblender outputs.
- measRecord
lsst.afw.table.SourceRecord Record describing the object being measured. Previously-measured quantities will be retrieved from here, and it will be updated in-place with the outputs of this plugin.
- refRecord
lsst.afw.table.SimpleRecord Additional parameters to define the fit, as measured elsewhere.
- refWcs
lsst.afw.geom.SkyWcsorlsst.afw.geom.Angle The coordinate system for the reference catalog values. An
Anglemay be passed, indicating that a local tangent WCS should be created for each object using the given angle as a pixel scale.
Notes#
In the normal mode of operation, the source centroid will be set to the WCS-transformed position of the reference object, so plugins that only require a reference position should not have to access the reference object at all.
- exposure
- config