An introduction to Bayesian inference in gravitational-wave astronomy: Parameter estimation, model selection, and hierarchical models

被引:319
作者
Thrane, Eric [1 ]
Talbot, Colm [2 ]
机构
[1] Monash Univ, Sch Phys & Astron, Ctr Astrophys, Clayton, Vic 3800, Australia
[2] OzGrav ARC Ctr Excellence Gravitat Wave Discovery, Clayton, Vic 3800, Australia
来源
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA | 2019年 / 36卷
基金
澳大利亚研究理事会;
关键词
methods: statistical; gravitational waves; stars: black holes; stars: neutron;
D O I
10.1017/pasa.2019.2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This is an introduction to Bayesian inference with a focus on hierarchical models and hyper-parameters. We write primarily for an audience of Bayesian novices, but we hope to provide useful insights for seasoned veterans as well. Examples are drawn from gravitational-wave astronomy, though we endeavour for the presentation to be understandable to a broader audience. We begin with a review of the fundamentals: likelihoods, priors, and posteriors. Next, we discuss Bayesian evidence, Bayes factors, odds ratios, and model selection. From there, we describe how posteriors are estimated using samplers such as Markov Chain Monte Carlo algorithms and nested sampling. Finally, we generalise the formalism to discuss hyper-parameters and hierarchical models. We include extensive appendices discussing the creation of credible intervals, Gaussian noise, explicit marginalisation, posterior predictive distributions, and selection effects.
引用
收藏
页数:12
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