Bayesian estimation of pulsar parameters from gravitational wave data

Dupuis, R.J. and Woan, G. (2005) Bayesian estimation of pulsar parameters from gravitational wave data. Physical Review D, 72(10), p. 102002. (doi: 10.1103/PhysRevD.72.102002)

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Publisher's URL: http://dx.doi.org/10.1103/PhysRevD.72.102002

Abstract

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.

Item Type:Articles
Status:Published
Refereed:Yes
Glasgow Author(s) Enlighten ID:Woan, Professor Graham
Authors: Dupuis, R.J., and Woan, G.
Subjects:Q Science > QB Astronomy
Q Science > QC Physics
College/School:College of Science and Engineering > School of Physics and Astronomy
Journal Name:Physical Review D
Publisher:American Physical Society
ISSN:1550-7998
ISSN (Online):1089-4918

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