Bayesian estimation of pulsar parameters from gravitational wave data

Details Bayesian estimation of pulsar parameters from gravitational wave data Bayesian estimation of pulsar parameters from gravitational wave data

2005-08-23

arxiv.org/abs/gr-qc/0508096v2

Phys.Rev. D72 (2005) 102002

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

9 pages, 6 figures. Accepted to Phys. Rev. D. A few small changes from previous version

Scientific paper

We present a method of searching for, and parameterizing, 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 in the covariance between the signal parameters.

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