Authors
George Hobbs, A Archibald, Zaven Arzoumanian, D Backer, M Bailes, NDR Bhat, M Burgay, Sarah Burke-Spolaor, D Champion, Ismaël Cognard, William Coles, J Cordes, P Demorest, G Desvignes, Robert D Ferdman, L Finn, P Freire, M Gonzalez, J Hessels, Aidan Hotan, G Janssen, F Jenet, A Jessner, C Jordan, V Kaspi, Michael Kramer, V Kondratiev, J Lazio, K Lazaridis, KJ Lee, Yuri Levin, A Lommen, D Lorimer, R Lynch, A Lyne, Richard Manchester, M McLaughlin, David Nice, Stefan Oslowski, M Pilia, A Possenti, M Purver, Scott Ransom, J Reynolds, S Sanidas, John Sarkissian, A Sesana, R Shannon, Xavier Siemens, I Stairs, B Stappers, D Stinebring, G Theureau, Rutger van Haasteren, Willem van Straten, JPW Verbiest, DRB Yardley, XP You
Publication date
2010/4/6
Journal
Classical and Quantum Gravity
Volume
27
Issue
8
Pages
084013
Publisher
IOP Publishing
Description
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.
Total citations
Scholar articles
G Hobbs, A Archibald, Z Arzoumanian, D Backer… - Classical and Quantum Gravity, 2010