Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/12483
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Type: Journal article
Title: Second-generation laser interferometry for gravitational wave detection: ACIGA progress
Author: McClelland, D.
Scott, S.
Gray, M.
Shaddock, D.
Slagmolen, B.
Searle, A.
Blair, D.
Ju, L.
Winterflood, J.
Benabid, F.
Baker, M.
Munch, J.
Veitch, P.
Hamilton, M.
Ostermeyer, M.
Mudge, D.
Ottaway, D.
Hollitt, C.
Citation: Classical and Quantum Gravity, 2001; 18(19):4121-4126
Publisher: IOP Publishing Ltd
Issue Date: 2001
ISSN: 0264-9381
1361-6382
Statement of
Responsibility: 
D E McClelland, S M Scott, M B Gray, D A Shaddock, B J Slagmolen, A Searle, D G Blair, L Ju, J Winterflood, F Benabid, M Baker, J Munch, P J Veitch, M W Hamilton, M Ostermeyer, D Mudge, D Ottaway and C Hollitt
Abstract: Reasonable event rate gravitational wave astronomy in the audio frequency detection band will require improving the sensitivity of long-baseline interferometer-based gravitational wave detectors currently under construction by at least a factor of 10. In this summary we report research being carried out by the Australian Consortium for Interferometric Gravitational Astronomy towards this end.
Rights: © 2001 IOP Publishing
RMID: 0020010417
DOI: 10.1088/0264-9381/18/19/321
Published version: http://www.iop.org/EJ/abstract/0264-9381/18/19/321/
Appears in Collections:Physics publications
Environment Institute publications

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