MeasureMergedDcrCoaddSourcesTask¶
Python API summary¶
from lsst.pipe.tasks.dcrMultiBand import MeasureMergedDcrCoaddSourcesTask
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class
(butler=None, schema=None, peakSchema=None, refObjLoader=None, initInputs=None, **kwargs)MeasureMergedDcrCoaddSourcesTask
Deblend sources from master catalog in each coadd seperately and measure
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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, sourceTableHandleDict=None, finalizedSourceTableHandleDict=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 MeasureMergedDcrCoaddSourcesTask
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.propagateSourceFlags.PropagateSourceFlagsTask
- Field type
ConfigurableField
Propagate source 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
doAddFootprints¶
Whether or not to add footprints to the input catalog from scarlet models. This should be true whenever using the multi-band deblender, otherwise this should be False.
doConserveFlux¶
Whether to use the deblender models as templates to re-distribute the flux from the ‘exposure’ (True), or to perform measurements on the deblender model footprints.
doPropagateFlags¶
Whether to match sources to CCD catalogs to propagate flags (to e.g. identify PSF stars)
doStripFootprints¶
Whether to strip footprints from the output catalog before saving to disk. This is usually done when using scarlet models to save disk space.
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¶
- Default
'deblendedCatalog'
- Field type
str
ChoiceField
(optional)- Choices
'deblendedCatalog'
- Output catalog from ScarletDeblendTask
'deblendedFlux'
- Output catalog from SourceDeblendTask
'mergeDet'
- The merged detections before deblending.
None
- Field is optional
The name of the input catalog.
saveLogOutput¶
Flag to enable/disable saving of log output for a task, enabled by default.