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| doMagLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply magnitude limit?") |
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| doFlags = pexConfig.Field(dtype=bool, default=False, doc="Apply flag limitation?") |
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| doUnresolved = pexConfig.Field(dtype=bool, default=False, doc="Apply unresolved limitation?") |
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| doSignalToNoise = pexConfig.Field(dtype=bool, default=False, doc="Apply signal-to-noise limit?") |
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| doMagError = pexConfig.Field(dtype=bool, default=False, doc="Apply magnitude error limit?") |
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| magLimit = pexConfig.ConfigField(dtype=MagnitudeLimit, doc="Magnitude limit to apply") |
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| flags = pexConfig.ConfigField(dtype=RequireFlags, doc="Flags to require") |
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| unresolved = pexConfig.ConfigField(dtype=RequireUnresolved, doc="Star/galaxy separation to apply") |
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| signalToNoise = pexConfig.ConfigField(dtype=SignalToNoiseLimit, doc="Signal-to-noise limit to apply") |
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| magError = pexConfig.ConfigField(dtype=MagnitudeErrorLimit, doc="Magnitude error limit to apply") |
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| colorLimits |
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Definition at line 605 of file sourceSelector.py.
◆ colorLimits
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.colorLimits |
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static |
Initial value:= pexConfig.ConfigDictField(keytype=str, itemtype=ColorLimit, default={},
doc="Color limits to apply; key is used as a label only")
Definition at line 616 of file sourceSelector.py.
◆ doFlags
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doFlags = pexConfig.Field(dtype=bool, default=False, doc="Apply flag limitation?") |
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static |
◆ doMagError
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doMagError = pexConfig.Field(dtype=bool, default=False, doc="Apply magnitude error limit?") |
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static |
◆ doMagLimit
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doMagLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply magnitude limit?") |
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static |
◆ doSignalToNoise
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doSignalToNoise = pexConfig.Field(dtype=bool, default=False, doc="Apply signal-to-noise limit?") |
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static |
◆ doUnresolved
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doUnresolved = pexConfig.Field(dtype=bool, default=False, doc="Apply unresolved limitation?") |
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◆ flags
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.flags = pexConfig.ConfigField(dtype=RequireFlags, doc="Flags to require") |
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◆ magError
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.magError = pexConfig.ConfigField(dtype=MagnitudeErrorLimit, doc="Magnitude error limit to apply") |
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◆ magLimit
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.magLimit = pexConfig.ConfigField(dtype=MagnitudeLimit, doc="Magnitude limit to apply") |
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static |
◆ signalToNoise
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.signalToNoise = pexConfig.ConfigField(dtype=SignalToNoiseLimit, doc="Signal-to-noise limit to apply") |
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static |
◆ unresolved
lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.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: