期刊
CLASSICAL AND QUANTUM GRAVITY
卷 27, 期 8, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/27/8/084014
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- STFC [ST/G002487/1, ST/F002874/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/F002874/1, ST/G002487/1] Funding Source: researchfish
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.
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