The European Pulsar Timing Array: current efforts and a LEAP toward the future

R. D. Ferdman, R. van Haasteren, C. G. Bassa, M. Burgay, I. Cognard, A. Corongiu, N. D'Amico, G. Desvignes, J. W. T. Hessels, G. H. Janssen, A. Jessner, C. Jordan, R. Karuppusamy, E. F. Keane, M. Kramer, K. Lazaridis, Y. Levin, A. G. Lyne, M. Pilia, A. PossentiM. Purver, B. Stappers, S. Sanidas, R. Smits, G. Theureau

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Abstract

The European Pulsar Timing Array (EPTA) is a multi-institutional, multi-telescope collaboration, with the goal of using high-precision pulsar timing to directly detect gravitational waves. In this paper we discuss the EPTA member telescopes, current achieved timing precision and near-future goals. We report a preliminary upper limit to the amplitude of a gravitational wave background. We also discuss the Large European Array for Pulsars, in which the five major European telescopes involved in pulsar timing will be combined to provide a coherent array that will give similar sensitivity to the Arecibo radio telescope, and larger sky coverage.

Original languageEnglish
Article number084014
Number of pages10
JournalClassical and Quantum Gravity
Volume27
Issue number8
DOIs
Publication statusPublished - 21 Apr 2010
Externally publishedYes
Event8th Edoardo Amaldi Conference on Gravitational Waves - New York
Duration: 22 Jun 200926 Jun 2009

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