Parameter estimation of spinning binary inspirals using Markov chain Monte Carlo

被引：90

作者：

van der Sluys, Marc ^{[1
]}

Raymond, Vivien ^{[1
,2
]}

Mandel, Ilya ^{[1
]}

Roever, Christian ^{[3
,4
]}

Christensen, Nelson ^{[5
]}

Kalogera, Vicky ^{[1
]}

Meyer, Renate ^{[3
]}

Vecchio, Alberto ^{[1
,6
]}

机构：

[1] Northwestern Univ, Dept Phys & Astron, Evanston, IL 60208 USA

[2] Univ Strasbourg, Strasbourg, France

[3] Univ Auckland, Dept Stat, Auckland 1, New Zealand

[4] Max Planck Inst Gravitat Phys, Hannover, Germany

[5] Carleton Coll, Dept Phys & Astron, Northfield, MN 55057 USA

[6] Univ Birmingham, Dept Phys & Astron, Birmingham, W Midlands, England

来源：

CLASSICAL AND QUANTUM GRAVITY | 2008年 / 25卷 / 18期

基金：

英国科学技术设施理事会;

关键词：

D O I：

10.1088/0264-9381/25/18/184011

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a Markov chain Monte Carlo (MCMC) technique to study the source parameters of gravitational-wave signals from the inspirals of stellarmass compact binaries detected with ground-based gravitational-wave detectors such as LIGO and Virgo, for the case where spin is present in the more massive compact object in the binary. We discuss the aspects of the MCMC algorithm that allowus to sample the parameter space in an efficientway. We show sample runs that illustrate the possibilities of our MCMC code and the difficulties that we encounter.

引用

页数：10

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