A Bayesian parameter estimation approach to pulsar time-of-arrival analysis

Messenger, C. , Lommen, A., Demorest, P. and Ransom, S. (2011) A Bayesian parameter estimation approach to pulsar time-of-arrival analysis. Classical and Quantum Gravity, 28(5), 055001. (doi:10.1088/0264-9381/28/5/055001)

Full text not currently available from Enlighten.


The increasing sensitivities of pulsar timing arrays to ultra-low frequency (nHz) gravitational waves promise to achieve direct gravitational wave (GW) detection within the next 5–10 years. While there are many parallel efforts being made in the improvement of telescope sensitivity, the detection of stable millisecond pulsars and the improvement of the timing software, there are reasons to believe that the methods used to accurately determine the time-of-arrival (TOA) of pulses from radio pulsars can be improved upon. More specifically, the determination of the uncertainties on these TOAs, which strongly affect the ability to detect GWs through pulsar timing, may be unreliable. We propose two Bayesian methods for the generation of pulsar TOAs starting from pulsar 'search-mode' data and pre-folded data. These methods are applied to simulated toy-model examples and in this initial work we focus on the issue of uncertainties in the folding period. The final results of our analysis are expressed in the form of posterior probability distributions on the signal parameters (including the TOA) from a single observation.

Item Type:Articles
Glasgow Author(s) Enlighten ID:Messenger, Dr Christopher
Authors: Messenger, C., Lommen, A., Demorest, P., and Ransom, S.
College/School:College of Science and Engineering > School of Physics and Astronomy
Journal Name:Classical and Quantum Gravity
Publisher:Institute of Physics Publishing Ltd.
ISSN (Online):1361-6382

University Staff: Request a correction | Enlighten Editors: Update this record