BEAST-Fitting / megabeast

Hierarchical Bayesian Model for Ensembles of Dust Extinguished Stellar Populations
http://megabeast.readthedocs.io/
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Completeness specific to source density #49

Open karllark opened 4 years ago

karllark commented 4 years ago

The completeness is a function of source density. The current implementation only allows for a single noise model, hence source density. This should be generalized. Either by using the stats file to get the reorder_tag (I think) to say which noise model to use, or get add this info to the lnp file when reordering the BEAST results.