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