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Unified population inference

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[![Build Status](https://travis-ci.com/ColmTalbot/gwpopulation.svg?branch=master)](https://travis-ci.com/ColmTalbot/gwpopulation) [![Maintainability](https://api.codeclimate.com/v1/badges/579536603e8e06466e63/maintainability)](https://codeclimate.com/github/ColmTalbot/gwpopulation/maintainability) [![Test Coverage](https://api.codeclimate.com/v1/badges/579536603e8e06466e63/test_coverage)](https://codeclimate.com/github/ColmTalbot/gwpopulation/test_coverage)

A collection of parametric binary black hole mass/spin population models.

Warning: This is under _very_ active development. No guarantee of backward compatibility is guaranteed.

These are formatted to be consistent with the [Bilby](https://git.ligo.org/lscsoft/bilby) [hyper-parameter inference package](https://lscsoft.docs.ligo.org/bilby/hyperparameters.html).

Most of the models implemented are derived from models presented in one of: - [Talbot & Thrane (2017)](https://arxiv.org/abs/1704.08370) - [Talbot & Thrane (2018)](https://arxiv.org/abs/1801.02699) - [Wysocki et al. (2018)](https://arxiv.org/abs/1805.06442) - [Fishbach et al. (2019)](https://arxiv.org/abs/1805.10270)

Automatically generated docs can be found [here](https://colm.talbot.docs.ligo.org/population/).

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