ScienceSourceSelectorTask¶
ScienceSourceSelectorTask selects sources from images being processed by optionally applying magnitude limits, flag requirements and star/galaxy separation.
Python API summary¶
from lsst.meas.algorithms.sourceSelector import ScienceSourceSelectorTask
- 
class
ScienceSourceSelectorTask(**kwargs) Science source selector
...
- attributeconfig
 Access configuration fields and retargetable subtasks.
- 
method
run(sourceCat, sourceSelectedField=None, matches=None, exposure=None) Select sources and return them
...
See also
See the ScienceSourceSelectorTask API reference for complete details.
Retargetable subtasks¶
No subtasks.
Configuration fields¶
doFlags¶
Apply flag limitation?
doFluxLimit¶
Apply flux limit?
doIsolated¶
Apply isolated limitation?
doRequireFiniteRaDec¶
Apply finite sky coordinate check?
doRequirePrimary¶
Apply source is primary check?
doSignalToNoise¶
Apply signal-to-noise limit?
doUnresolved¶
Apply unresolved limitation?
flags¶
- Data type
 lsst.meas.algorithms.sourceSelector.RequireFlags- Field type
 
Flags to require
fluxLimit¶
- Data type
 lsst.meas.algorithms.sourceSelector.FluxLimit- Field type
 
Flux limit to apply
isolated¶
- Data type
 lsst.meas.algorithms.sourceSelector.RequireIsolated- Field type
 
Isolated criteria to apply
requireFiniteRaDec¶
- Data type
 lsst.meas.algorithms.sourceSelector.RequireFiniteRaDec- Field type
 
Finite sky coordinate criteria to apply
requirePrimary¶
- Data type
 lsst.meas.algorithms.sourceSelector.RequirePrimary- Field type
 
Primary source criteria to apply
signalToNoise¶
- Data type
 lsst.meas.algorithms.sourceSelector.SignalToNoiseLimit- Field type
 
Signal-to-noise limit to apply
unresolved¶
- Data type
 lsst.meas.algorithms.sourceSelector.RequireUnresolved- Field type
 
Star/galaxy separation to apply