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

Authors
  • R.D. Ferdman
  • R. van Haasteren
  • C.G. Bassa
  • M. Burgay
Publication date 2010
Journal Classical and Quantum Gravity
Volume | Issue number 27 | 8
Pages (from-to) 084014
Number of pages 10
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
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.
Document type Article
Note ID: 533
Language English
Published at https://doi.org/10.1088/0264-9381/27/8/084014
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