The International Pulsar Timing Array project: Using pulsars as a gravitational wave detector

George Hobbs, A Archibald, Z Arzoumanian, D Backer, M Bailes, N D R Bhat, M Burgay, Sarah Burke-Spolaor, D Champion, I Cognard, William Coles, J Cordes, P Demorest, G Desvignes, R D Ferdman, L Finn, P Freire, M Gonzalez, J Hessels, A HotanG Janssen, F Jenet, A Jessner, C Jordan, V Kaspi, Michael Kramer, V Kondratiev, T Lazio, K Lazaridis, Kejia 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, J Verbiest, D Yardley, X You

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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 languageEnglish
Pages (from-to)1 - 10
Number of pages10
JournalClassical and Quantum Gravity
Issue number8
Publication statusPublished - 2010
Externally publishedYes

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