The sensitivity of the Parkes Pulsar Timing Array to individual sources of gravitational waves

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The sensitivity of the Parkes Pulsar Timing Array to individual sources of gravitational waves

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 m...

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Bibliographic Details
Main Authors:	Yardley, D., Hobbs, G., Jenet, F., Verbiest, J., Wen, Z., Manchester, R. N., Coles, W. A., van Straten, W., Bailes, M., Bhat, N. D. R., Burke-Spolaor, S., Champion, D. J., Hotan, Aidan, Sarkissian, J. M.
Format:	Journal Article
Published:	Wiley-Blackwell Publishing Ltd. 2010
Subjects:	methods data analysis gravitational waves pulsars: general galaxies: evolution
Online Access:	http://hdl.handle.net/20.500.11937/20234

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