McClelland, D. E.; Scott, S. M.; Gray, M. B.; Shaddock, D. A.; Slagmolen, B. J.; Searle, A.; Blair, D. G.; Ju, L.; Winterflood, J.; Benabid, F.; Baker, M.; Munch, J.; Veitch, P. J.; Hamilton, M. W.; Ostermeyer, M.; Mudge, D.; Ottaway, D.; Hollitt, C. Second-generation laser interferometry for gravitational wave detection: ACIGA progress. (English) Zbl 0991.83509 Classical Quantum Gravity 18, No. 19, 4121-4126 (2001). Summary: 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. Cited in 1 Document MSC: 83B05 Observational and experimental questions in relativity and gravitational theory 83C35 Gravitational waves Keywords:laser interferometry; gravitational wave PDFBibTeX XMLCite \textit{D. E. McClelland} et al., Classical Quantum Gravity 18, No. 19, 4121--4126 (2001; Zbl 0991.83509) Full Text: DOI