MeasureMergedCoaddSourcesTask¶
Python API summary¶
from lsst.pipe.tasks.multiBand import MeasureMergedCoaddSourcesTask
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class
(butler=None, schema=None, peakSchema=None, refObjLoader=None, initInputs=None, **kwargs)MeasureMergedCoaddSourcesTask
! @anchor MeasureMergedCoaddSourcesTask_
...
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attribute
config
Access configuration fields and retargetable subtasks.
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method
(exposure, sources, skyInfo, exposureId, ccdInputs=None, visitCatalogs=None, wcsUpdates=None, butler=None)run
Run measurement algorithms on the input exposure, and optionally populate the resulting catalog with extra information
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method
(patchRef, psfCache=100)runDataRef
! @brief Deblend and measure
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See also
See the MeasureMergedCoaddSourcesTask
API reference for complete details.
Retargetable subtasks¶
applyApCorr¶
- Default
lsst.meas.base.applyApCorr.ApplyApCorrTask
- Field type
ConfigurableField
Subtask to apply aperture corrections
catalogCalculation¶
- Default
lsst.meas.base.catalogCalculation.CatalogCalculationTask
- Field type
ConfigurableField
Subtask to run catalogCalculation plugins on catalog
match¶
- Default
lsst.meas.astrom.directMatch.DirectMatchTask
- Field type
ConfigurableField
Matching to reference catalog
measurement¶
- Default
lsst.meas.base.sfm.SingleFrameMeasurementTask
- Field type
ConfigurableField
Source measurement
propagateFlags¶
- Default
lsst.pipe.tasks.propagateVisitFlags.PropagateVisitFlagsTask
- Field type
ConfigurableField
Propagate visit flags to coadd
setPrimaryFlags¶
- Default
lsst.pipe.tasks.setPrimaryFlags.SetPrimaryFlagsTask
- Field type
ConfigurableField
Set flags for primary tract/patch
Configuration fields¶
checkUnitsParseStrict¶
Strictness of Astropy unit compatibility check, can be ‘raise’, ‘warn’ or ‘silent’
connections¶
- Data type
lsst.pipe.base.config.Connections
- Field type
ConfigField
Configurations describing the connections of the PipelineTask to datatypes
doPropagateFlags¶
Whether to match sources to CCD catalogs to propagate flags (to e.g. identify PSF stars)
doWriteMatchesDenormalized¶
Write reference matches in denormalized format? This format uses more disk space, but is more convenient to read.
hasFakes¶
Should be set to True if fake sources have been inserted into the input data.
inputCatalog¶
Name of the input catalog to use.If the single band deblender was used this should be ‘deblendedFlux.If the multi-band deblender was used this should be ‘deblendedModel.If no deblending was performed this should be ‘mergeDet’