lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig Class Reference

Inheritance diagram for lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig:

Public Member Functions
	setDefaults (self)

Static Public Attributes
	doFluxLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply flux limit?")
	doFlags = pexConfig.Field(dtype=bool, default=False, doc="Apply flag limitation?")
	doUnresolved = pexConfig.Field(dtype=bool, default=False, doc="Apply unresolved limitation?")
	doSignalToNoise = pexConfig.Field(dtype=bool, default=False, doc="Apply signal-to-noise limit?")
	doIsolated = pexConfig.Field(dtype=bool, default=False, doc="Apply isolated limitation?")
	doRequireFiniteRaDec
	doRequirePrimary
	doSkySources
	doCentroidErrorLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply limit on centroid errors?")
	fluxLimit = pexConfig.ConfigField(dtype=FluxLimit, doc="Flux limit to apply")
	flags = pexConfig.ConfigField(dtype=RequireFlags, doc="Flags to require")
	unresolved = pexConfig.ConfigField(dtype=RequireUnresolved, doc="Star/galaxy separation to apply")
	signalToNoise = pexConfig.ConfigField(dtype=SignalToNoiseLimit, doc="Signal-to-noise limit to apply")
	isolated = pexConfig.ConfigField(dtype=RequireIsolated, doc="Isolated criteria to apply")
	requireFiniteRaDec
	requirePrimary
	skyFlag = pexConfig.ConfigField(dtype=RequireFlags, doc="Sky source flag to include")
	centroidErrorLimit

Detailed Description

Configuration for selecting science sources

Definition at line 678 of file sourceSelector.py.

Member Function Documentation

setDefaults()

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.setDefaults

(

self

)

Definition at line 705 of file sourceSelector.py.

Member Data Documentation

centroidErrorLimit

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.centroidErrorLimit

static

Initial value:

=  pexConfig.ConfigField(dtype=CentroidErrorLimit,
                                               doc="Limit to place on centroid errors.")

Definition at line 702 of file sourceSelector.py.

doCentroidErrorLimit

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doCentroidErrorLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply limit on centroid errors?")

static

Definition at line 691 of file sourceSelector.py.

doFlags

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doFlags = pexConfig.Field(dtype=bool, default=False, doc="Apply flag limitation?")

static

Definition at line 681 of file sourceSelector.py.

doFluxLimit

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doFluxLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply flux limit?")

static

Definition at line 680 of file sourceSelector.py.

doIsolated

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doIsolated = pexConfig.Field(dtype=bool, default=False, doc="Apply isolated limitation?")

static

Definition at line 684 of file sourceSelector.py.

doRequireFiniteRaDec

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doRequireFiniteRaDec

static

Initial value:

=  pexConfig.Field(dtype=bool, default=False,
                                           doc="Apply finite sky coordinate check?")

Definition at line 685 of file sourceSelector.py.

doRequirePrimary

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doRequirePrimary

static

Initial value:

=  pexConfig.Field(dtype=bool, default=False,
                                       doc="Apply source is primary check?")

Definition at line 687 of file sourceSelector.py.

doSignalToNoise

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doSignalToNoise = pexConfig.Field(dtype=bool, default=False, doc="Apply signal-to-noise limit?")

static

Definition at line 683 of file sourceSelector.py.

doSkySources

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doSkySources

static

Initial value:

=  pexConfig.Field(dtype=bool, default=False,
                                   doc="Include sky sources, unioned with all other criteria?")

Definition at line 689 of file sourceSelector.py.

doUnresolved

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doUnresolved = pexConfig.Field(dtype=bool, default=False, doc="Apply unresolved limitation?")

static

Definition at line 682 of file sourceSelector.py.

flags

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.flags = pexConfig.ConfigField(dtype=RequireFlags, doc="Flags to require")

static

Definition at line 693 of file sourceSelector.py.

fluxLimit

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.fluxLimit = pexConfig.ConfigField(dtype=FluxLimit, doc="Flux limit to apply")

static

Definition at line 692 of file sourceSelector.py.

isolated

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.isolated = pexConfig.ConfigField(dtype=RequireIsolated, doc="Isolated criteria to apply")

static

Definition at line 696 of file sourceSelector.py.

requireFiniteRaDec

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.requireFiniteRaDec

static

Initial value:

=  pexConfig.ConfigField(dtype=RequireFiniteRaDec,
                                               doc="Finite sky coordinate criteria to apply")

Definition at line 697 of file sourceSelector.py.

requirePrimary

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.requirePrimary

static

Initial value:

=  pexConfig.ConfigField(dtype=RequirePrimary,
                                           doc="Primary source criteria to apply")

Definition at line 699 of file sourceSelector.py.

signalToNoise

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.signalToNoise = pexConfig.ConfigField(dtype=SignalToNoiseLimit, doc="Signal-to-noise limit to apply")

static

Definition at line 695 of file sourceSelector.py.

skyFlag

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.skyFlag = pexConfig.ConfigField(dtype=RequireFlags, doc="Sky source flag to include")

static

Definition at line 701 of file sourceSelector.py.

unresolved

lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.unresolved = pexConfig.ConfigField(dtype=RequireUnresolved, doc="Star/galaxy separation to apply")

static

Definition at line 694 of file sourceSelector.py.

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The documentation for this class was generated from the following file:

• python/lsst/meas/algorithms/sourceSelector.py