gwkokab.analysis.multisourceΒΆ
The multi-source analysis family.
A mixture over four kinds of mass component, meant to describe a population drawn from several astrophysical formation channels at once:
splβ smoothed power law primary mass with a conditional mass ratio power law;bplβ smoothed broken power law, same conditional mass ratio;gplβ Gaussian primary mass, same conditional mass ratio;ggβ independent truncated normals on \(m_1\) and \(m_2\).
Each component carries its own log rate, log_rate_<index>, indexed across the whole
mixture β one rate per channel.
Console scriptsΒΆ
discrete_multisourceβ infer the population from per-event posterior samples.analytical_gwalk_multisourceβ infer it from per-event Gaussian summaries.
The sampler backend is chosen at runtime by sampler_cfg.json, not by the entry point.
See also
gwkokab.models.hybrids.MultiSourceModelThe population model this family fits.
gwkokab.analysis.subpopulationThe same component families, but mixed at the level of the primary mass.