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 language | English |
|---|---|
| Article number | 084014 |
| Journal | Classical and Quantum Gravity |
| Volume | 27 |
| Issue number | 8 |
| DOIs | |
| Publication status | Published - 2010 |
| Externally published | Yes |