Search Swinburne Research Bank
Home List of Titles The sensitivity of the Parkes Pulsar Timing Array to individual sources of gravitational waves
Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.3/92840
|Download PDF (Accepted manuscript) (Adobe Acrobat PDF, 683 KB)|
- The sensitivity of the Parkes Pulsar Timing Array to individual sources of gravitational waves
- Yardley, D. R. B.; Hobbs, G. B.; Jenet, F. A.; Verbiest, J. P. W.; Wen, Z. L.; Manchester, R. N.; Coles, W. A.; van Straten, W.; Bailes, M.; Bhat, N. D. R.; Burke-Spolaor, S.; Champion, D. J.; Hotan, A. W.; Sarkissian, J. M.
- We present the sensitivity of the Parkes Pulsar Timing Array to gravitational waves (GWs) emitted by individual supermassive black hole binary systems in the early phases of coalescing at the cores of merged galaxies. Our analysis includes a detailed study of the effects of fitting a pulsar timing model to non-white timing residuals. Pulsar timing is sensitive at nanoHertz frequencies and hence complementary to Laser Interferometer Gravitational-Wave Observatory and Laser Interferometer Space Antenna. We place a sky-averaged constraint on the merger rate of nearby (z > 0.6) black hole binaries in the early phases of coalescence with a chirp mass of 10^10 M(.) of less than one merger every 7 yr. The prospects for future GW astronomy of this type with the proposed Square Kilometre Array telescope are discussed.
- Publication type
- Journal article
- Research centre
- Swinburne University of Technology. Faculty of Information and Communication Technologies. Centre for Astrophysics and Supercomputing
- Monthly Notices of the Royal Astronomical Society, Vol. 407, no. 1 (Sep 2010), pp. 669-680
- Publication year
- FOR Code(s)
- 0201 Astronomical and Space Sciences
- Data analysis methods; Galactic evolution; Gravitational waves; Parkes Pulsar Timing Array; Pulsars
- Publisher URL
- Copyright © 2010 The Authors. Journal compilation copyright © 2010 Royal Astronomical Society. The accepted manuscript of this paper is reproduced here in accordance with the copyright policy of the publisher. The definitive publication is available at www.interscience.wiley.com.
- Research Projects
- Full text
- Peer reviewed