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

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

Internet

http://hdl.handle.net/20.500.11937/20234

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