Abstract
The International Pulsar Timing Array project combines observations of pulsars from both northern and southern hemisphere observatories with the main aim of detecting ultra-low frequency (∼ 10-9-10-8 Hz) gravitational waves. Here we introduce the project, review the methods used to search for gravitational waves emitted from coalescing supermassive binary black-hole systems in the centres of merging galaxies and discuss the status of the project.
Original language | English (US) |
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Article number | 084013 |
Journal | Classical and Quantum Gravity |
Volume | 27 |
Issue number | 8 |
DOIs | |
State | Published - 2010 |
All Science Journal Classification (ASJC) codes
- Physics and Astronomy (miscellaneous)