def lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsTask.__init__ |
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self, |
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butler, |
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args, |
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kwargs |
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def lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsTask.get_shards |
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self, |
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id_list |
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Get all shards that touch a circular aperture.
- Parameters
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[in] | id_list | A list of integer pixel ids |
[out] | a | list of SourceCatalogs for each pixel, None if not data exists |
Definition at line 110 of file loadIndexedReferenceObjects.py.
def lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsTask.loadSkyCircle |
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self, |
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ctrCoord, |
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radius, |
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filterName = None |
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Load reference objects that overlap a circular sky region.
- Parameters
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[in] | ctrCoord | center of search region (an lsst.afw.geom.Coord) |
[in] | radius | radius of search region (an lsst.afw.geom.Angle) |
[in] | filterName | name of filter, or None for the default filter; used for flux values in case we have flux limits (which are not yet implemented) |
- Returns
- an lsst.pipe.base.Struct containing:
- refCat a catalog of reference objects with the standard schema as documented in LoadReferenceObjects, including photometric, resolved and variable; hasCentroid is False for all objects.
- fluxField = name of flux field for specified filterName. None if refCat is None.
Definition at line 58 of file loadIndexedReferenceObjects.py.
lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsTask.butler |
lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsTask.indexer |
lsst.meas.algorithms.loadIndexedReferenceObjects.LoadIndexedReferenceObjectsTask.ref_dataset_name |
The documentation for this class was generated from the following file: