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

Hobbs, G.; M. Archibald, Anne; Arzoumanian, Zaven; C. Backer, D.; Bailes, M.; D. R. Bhat, N.; Burgay, M.; Burke-Spolaor, Sarah; J. Champion, D.; Cognard, I.; A. Coles, W.; M. Cordes, J.; B. Demorest, Paul; Desvignes, G.; D. Ferdman, R.; S. Finn, L.; C. C. Freire, P.; Gonzalez, Marjorie; W. T. Hessels, J.; W. Hotan, A.; H. Janssen, G.; A. Jenet, F.; Jessner, A.; Jordan, C.; M. Kaspi, V.; Krämer, M.; I. Kondratiev, V.; Lazio, Joseph; Lazaridis, K.; J. Lee, K.; Levin, Y.; N. Lommen, A.; R. Lorimer, D.; S. Lynch, Ryan; G. Lyne, A.; N. Manchester, R.; A. McLaughlin, M.; J. Nice, David; Osłowski, S.; Pilia, M.; Possenti, Andrea; B. Purver, M.; M. Ransom, S.; E. Reynolds, J.; A. Sanidas, S.; Sarkissian, John; Sesana, Alberto; M. Shannon, R.; Siemens, Xavier; H. Stairs, I.; W. Stappers, B.; R. Stinebring, Daniel; Theureau, G.; van Haasteren, Rutger; van Straten, W.; P. W. Verbiest, J.; R. B. Yardley, D.; P. You, X.

doi:10.1088/0264-9381/27/8/084013

Public

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

Published in Classical and Quantum Gravity • Apr 6, 2010

Authors:

G. Hobbs

Anne M. Archibald

Zaven Arzoumanian

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 gra...

Subject

Physics

Pulsar

Gravitational wave

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