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 (similar to 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 |
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Article number | 084013 |
Number of pages | 10 |
Journal | Classical and Quantum Gravity |
Volume | 27 |
Issue number | 8 |
DOIs | |
Publication status | Published - 6 Apr 2010 |
Externally published | Yes |
Event | 8th Edoardo Amaldi Conference on Gravitational Waves - New York, United States Duration: 22 Jun 2009 → 26 Jun 2009 |