On detection of the stochastic gravitational-wave background using the Parkes pulsar timing array

On detection of the stochastic gravitational-wave background using the Parkes pulsar timing array

We search for the signature of an isotropic stochastic gravitational-wave background in pulsar timing observations using a frequency-domain correlation technique. These observations, which span roughly 12 yr, were obtained with the 64-m Parkes radio telescope augmented by public domain observations...

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Bibliographic Details
Main Authors: Yardley, D., Coles, W., Hobbs, G., Verbiest, J., Manchester R. N., van Straten W., Jenet F. A., Bailes M., Bhat, Ramesh, Burke-Spolaor, S., Champion, D. J., Hotan, Aidan, Oslowski, S., Reynolds, J. E., Sarkissian, J. M.
Format: Journal Article
Published: Wiley-Blackwell Publishing Ltd. 2011
Subjects:
gravitational waves
stars: pulsars: general
methods: data analysis
Online Access:http://hdl.handle.net/20.500.11937/13890

Internet

http://hdl.handle.net/20.500.11937/13890

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