LSST Applications  21.0.0-172-gfb10e10a+18fedfabac,22.0.0+297cba6710,22.0.0+80564b0ff1,22.0.0+8d77f4f51a,22.0.0+a28f4c53b1,22.0.0+dcf3732eb2,22.0.1-1-g7d6de66+2a20fdde0d,22.0.1-1-g8e32f31+297cba6710,22.0.1-1-geca5380+7fa3b7d9b6,22.0.1-12-g44dc1dc+2a20fdde0d,22.0.1-15-g6a90155+515f58c32b,22.0.1-16-g9282f48+790f5f2caa,22.0.1-2-g92698f7+dcf3732eb2,22.0.1-2-ga9b0f51+7fa3b7d9b6,22.0.1-2-gd1925c9+bf4f0e694f,22.0.1-24-g1ad7a390+a9625a72a8,22.0.1-25-g5bf6245+3ad8ecd50b,22.0.1-25-gb120d7b+8b5510f75f,22.0.1-27-g97737f7+2a20fdde0d,22.0.1-32-gf62ce7b1+aa4237961e,22.0.1-4-g0b3f228+2a20fdde0d,22.0.1-4-g243d05b+871c1b8305,22.0.1-4-g3a563be+32dcf1063f,22.0.1-4-g44f2e3d+9e4ab0f4fa,22.0.1-42-gca6935d93+ba5e5ca3eb,22.0.1-5-g15c806e+85460ae5f3,22.0.1-5-g58711c4+611d128589,22.0.1-5-g75bb458+99c117b92f,22.0.1-6-g1c63a23+7fa3b7d9b6,22.0.1-6-g50866e6+84ff5a128b,22.0.1-6-g8d3140d+720564cf76,22.0.1-6-gd805d02+cc5644f571,22.0.1-8-ge5750ce+85460ae5f3,master-g6e05de7fdc+babf819c66,master-g99da0e417a+8d77f4f51a,w.2021.48
LSST Data Management Base Package
Public Member Functions | Static Public Attributes | List of all members
lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig Class Reference
Inheritance diagram for lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig:

Public Member Functions

def 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?")
 
 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")
 

Detailed Description

Configuration for selecting science sources

Definition at line 487 of file sourceSelector.py.

Member Function Documentation

◆ setDefaults()

def lsst.meas.algorithms.sourceSelector.ScienceSourceSelectorConfig.setDefaults (   self)

Definition at line 500 of file sourceSelector.py.

500  def setDefaults(self):
501  pexConfig.Config.setDefaults(self)
502  self.flags.bad = ["base_PixelFlags_flag_edge", "base_PixelFlags_flag_saturated", "base_PsfFlux_flags"]
503  self.signalToNoise.fluxField = "base_PsfFlux_instFlux"
504  self.signalToNoise.errField = "base_PsfFlux_instFluxErr"
505 
506 
507 @pexConfig.registerConfigurable("science", sourceSelectorRegistry)

Member Data Documentation

◆ doFlags

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

Definition at line 490 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 489 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 493 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 492 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 491 of file sourceSelector.py.

◆ flags

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

Definition at line 495 of file sourceSelector.py.

◆ fluxLimit

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

Definition at line 494 of file sourceSelector.py.

◆ isolated

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

Definition at line 498 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 497 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 496 of file sourceSelector.py.


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