rail.interactive.estimation.algos.train_z module
- rail.interactive.estimation.algos.train_z.train_z_estimator(**kwargs)
CatEstimator which returns a global PDF for all galaxies
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The main interface method for the photo-z estimation
This will attach the input data (defined in
inputsas “input”) to thisEstimator(for introspection and provenance tracking). Then call therun(),validate(), andfinalize()methods.The run method will call
_process_chunk(), which needs to be implemented in the subclass, to process input data in batches. SeeRandomGaussEstimatorfor a simple example.Finally, this will return a
QPHandlefor access to that output data.—
This function was generated from the function rail.estimation.algos.train_z.TrainZEstimator.estimate
- Parameters:
input_data (TableLike, required) – A dictionary of all input data
model (numpy.ndarray, required)
chunk_size (int, optional) – Number of objects per chunk for parallel processing or to evalute per loop in single node processing Default: 10000
hdf5_groupname (str, optional) – name of hdf5 group for data, if None, then set to ‘’ Default: photometry
zmin (float, optional) – The minimum redshift of the z grid or sample Default: 0.0
zmax (float, optional) – The maximum redshift of the z grid or sample Default: 3.0
nzbins (int, optional) – The number of gridpoints in the z grid Default: 301
id_col (str, optional) – name of the object ID column Default: object_id
redshift_col (str, optional) – name of redshift column Default: redshift
calc_summary_stats (bool, optional) – Compute summary statistics Default: False
calculated_point_estimates (list, optional) – List of strings defining which point estimates to automatically calculate using qp.Ensemble.Options include, ‘mean’, ‘mode’, ‘median’. Default: []
recompute_point_estimates (bool, optional) – Force recomputation of point estimates Default: False
- Returns:
Handle providing access to QP ensemble with output data
- Return type:
qp.core.ensemble.Ensemble
- rail.interactive.estimation.algos.train_z.train_z_informer(**kwargs)
Train an Estimator which returns a global PDF for all galaxies
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The main interface method for Informers
This will attach the input_data to this Informer (for introspection and provenance tracking).
Then it will call the run(), validate() and finalize() methods, which need to be implemented by the sub-classes.
The run() method will need to register the model that it creates to this Estimator by using self.add_data(‘model’, model).
Finally, this will return a ModelHandle providing access to the trained model.
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This function was generated from the function rail.estimation.algos.train_z.TrainZInformer.inform
- Parameters:
training_data (TableLike, required) – dictionary of all input data, or a TableHandle providing access to it
hdf5_groupname (str, optional) – name of hdf5 group for data, if None, then set to ‘’ Default: photometry
zmin (float, optional) – The minimum redshift of the z grid or sample Default: 0.0
zmax (float, optional) – The maximum redshift of the z grid or sample Default: 3.0
nzbins (int, optional) – The number of gridpoints in the z grid Default: 301
redshift_col (str, optional) – name of redshift column Default: redshift
- Returns:
Handle providing access to trained model
- Return type:
numpy.ndarray