asimov-pastro

Integration between Asimov and Pastro for astrophysical parameter inference from gravitational wave posteriors.

Features

• Population analysis from single-event posteriors
• Astrophysical parameter inference beyond detector frame
• Bayesian hierarchical models for population studies
• Integration with asimov workflows

Installation

pip install asimov-pastro

Purpose

Pastro takes parameter estimation results and infers astrophysical population properties, such as merger rates, mass distributions, and other source characteristics that inform our understanding of compact object populations.

Documentation

• Pastro Documentation
• Population Analysis Guide

Status

Stable - Used in production catalogue analyses

Use Cases

• Population parameter inference from catalogues
• Astrophysical parameter extraction
• Mass distribution studies
• Binary black hole demographics