Bayesian estimation of pulsar parameters from gravitational wave data

被引：82

作者：

Dupuis, RJ ^{[1
]}

Woan, G

机构：

[1] CALTECH, Pasadena, CA 91125 USA

[2] Univ Glasgow, Glasgow G12 8QQ, Lanark, Scotland

来源：

PHYSICAL REVIEW D | 2005年 / 72卷 / 10期

关键词：

D O I：

10.1103/PhysRevD.72.102002

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a method of searching for, and parametrizing, signals from known radio pulsars in data from interferometric gravitational wave detectors. This method has been applied to data from the LIGO and GEO 600 detectors to set upper limits on the gravitational wave emission from several radio pulsars. Here we discuss the nature of the signal and the performance of the technique on simulated data. We show how to perform a coherent multiple detector analysis and give some insight into the covariance between the signal parameters.

引用

页数：9

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