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Gravitational-Wave Detection Using Pulsars: Status of the Parkes Pulsar Timing Array Project

G. B. Hobbs A J , M. Bailes B , N. D. R. Bhat B , S. Burke-Spolaor A B , D. J. Champion A , W. Coles C , A. Hotan D , F. Jenet E , L. Kedziora-Chudczer A , J. Khoo A , K. J. Lee E F , A. Lommen G , R. N. Manchester A , J. Reynolds A , J. Sarkissian A , W. van Straten B , S. To A H , J. P. W. Verbiest A B , D. Yardley A H and X. P. You I
+ Author Affiliations
- Author Affiliations

A Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping, NSW 1710

B Centre for Astrophysics and Supercomputing, Swinburne University of Technology, P.O. Box 218, Hawthorn, VIC 3122

C Electrical and Computer Engineering, University of California at San Diego, La Jolla, California, USA

D Department of Imaging and Applied Physics, Curtin University of Technology, P.O. Box U1987, Perth, WA 6845

E Center for Gravitational Wave Astronomy, University of Texas at Brownsville, 80 Fort Brown, Brownsville, TX 78520

F Department of Astronomy, Peking University, 5 Haidian Lu, Beijing 100871, China – PRC

G Franklin and Marshall College, 415 Harrisburg Pike, Lancaster, PA 17604, USA

H Institute of Astronomy, School of Physics A29, The University of Sydney, NSW 2006

I School of Physical Science and Technology, Southwest University, 2 Tiansheng Road, Chongqing 400715, China – PRC

J Corresponding author. Email: George.Hobbs@csiro.au

Publications of the Astronomical Society of Australia 26(2) 103-109 https://doi.org/10.1071/AS08023
Submitted: 30 September 2008  Accepted: 14 December 2008   Published: 26 June 2009



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