|
| | doMagLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply magnitude 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?") |
| |
| | doMagError = pexConfig.Field(dtype=bool, default=False, doc="Apply magnitude error limit?") |
| |
| | magLimit = pexConfig.ConfigField(dtype=MagnitudeLimit, doc="Magnitude 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") |
| |
| | magError = pexConfig.ConfigField(dtype=MagnitudeErrorLimit, doc="Magnitude error limit to apply") |
| |
| | colorLimits |
| |
Definition at line 550 of file sourceSelector.py.
◆ colorLimits
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.colorLimits |
|
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 561 of file sourceSelector.py.
◆ doFlags
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doFlags = pexConfig.Field(dtype=bool, default=False, doc="Apply flag limitation?") |
|
static |
◆ doMagError
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doMagError = pexConfig.Field(dtype=bool, default=False, doc="Apply magnitude error limit?") |
|
static |
◆ doMagLimit
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doMagLimit = pexConfig.Field(dtype=bool, default=False, doc="Apply magnitude limit?") |
|
static |
◆ doSignalToNoise
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doSignalToNoise = pexConfig.Field(dtype=bool, default=False, doc="Apply signal-to-noise limit?") |
|
static |
◆ doUnresolved
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.doUnresolved = pexConfig.Field(dtype=bool, default=False, doc="Apply unresolved limitation?") |
|
static |
◆ flags
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.flags = pexConfig.ConfigField(dtype=RequireFlags, doc="Flags to require") |
|
static |
◆ magError
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.magError = pexConfig.ConfigField(dtype=MagnitudeErrorLimit, doc="Magnitude error limit to apply") |
|
static |
◆ magLimit
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.magLimit = pexConfig.ConfigField(dtype=MagnitudeLimit, doc="Magnitude limit to apply") |
|
static |
◆ signalToNoise
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.signalToNoise = pexConfig.ConfigField(dtype=SignalToNoiseLimit, doc="Signal-to-noise limit to apply") |
|
static |
◆ unresolved
| lsst.meas.algorithms.sourceSelector.ReferenceSourceSelectorConfig.unresolved = pexConfig.ConfigField(dtype=RequireUnresolved, doc="Star/galaxy separation to apply") |
|
static |
The documentation for this class was generated from the following file: