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pexConfig | doFluxLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply flux limit?") |
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pexConfig | doFlags = pexConfig.Field(dtype=bool, default=False, doc="Apply flag limitation?") |
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pexConfig | doUnresolved = pexConfig.Field(dtype=bool, default=False, doc="Apply unresolved limitation?") |
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pexConfig | doSignalToNoise = pexConfig.Field(dtype=bool, default=False, doc="Apply signal-to-noise limit?") |
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pexConfig | doIsolated = pexConfig.Field(dtype=bool, default=False, doc="Apply isolated limitation?") |
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pexConfig | doRequireFiniteRaDec |
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pexConfig | fluxLimit = pexConfig.ConfigField(dtype=FluxLimit, doc="Flux limit to apply") |
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pexConfig | flags = pexConfig.ConfigField(dtype=RequireFlags, doc="Flags to require") |
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pexConfig | unresolved = pexConfig.ConfigField(dtype=RequireUnresolved, doc="Star/galaxy separation to apply") |
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pexConfig | signalToNoise = pexConfig.ConfigField(dtype=SignalToNoiseLimit, doc="Signal-to-noise limit to apply") |
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pexConfig | isolated = pexConfig.ConfigField(dtype=RequireIsolated, doc="Isolated criteria to apply") |
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pexConfig | requireFiniteRaDec |
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Configuration for selecting science sources
Definition at line 527 of file sourceSelector.py.
◆ setDefaults()
def lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.setDefaults |
( |
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self | ) |
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◆ doFlags
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doFlags = pexConfig.Field(dtype=bool, default=False, doc="Apply flag limitation?") |
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◆ doFluxLimit
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doFluxLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply flux limit?") |
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◆ doIsolated
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doIsolated = pexConfig.Field(dtype=bool, default=False, doc="Apply isolated limitation?") |
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◆ doRequireFiniteRaDec
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doRequireFiniteRaDec |
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Initial value:= pexConfig.Field(dtype=bool, default=False,
doc="Apply finite sky coordinate check?")
Definition at line 534 of file sourceSelector.py.
◆ doSignalToNoise
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doSignalToNoise = pexConfig.Field(dtype=bool, default=False, doc="Apply signal-to-noise limit?") |
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◆ doUnresolved
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.doUnresolved = pexConfig.Field(dtype=bool, default=False, doc="Apply unresolved limitation?") |
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◆ flags
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.flags = pexConfig.ConfigField(dtype=RequireFlags, doc="Flags to require") |
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◆ fluxLimit
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.fluxLimit = pexConfig.ConfigField(dtype=FluxLimit, doc="Flux limit to apply") |
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◆ isolated
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.isolated = pexConfig.ConfigField(dtype=RequireIsolated, doc="Isolated criteria to apply") |
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◆ requireFiniteRaDec
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.requireFiniteRaDec |
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Initial value:= pexConfig.ConfigField(dtype=RequireFiniteRaDec,
doc="Finite sky coordinate criteria to apply")
Definition at line 541 of file sourceSelector.py.
◆ signalToNoise
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.signalToNoise = pexConfig.ConfigField(dtype=SignalToNoiseLimit, doc="Signal-to-noise limit to apply") |
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◆ unresolved
pexConfig lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.unresolved = pexConfig.ConfigField(dtype=RequireUnresolved, doc="Star/galaxy separation to apply") |
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static |
The documentation for this class was generated from the following file: