De. Mcclelland et al., Second-generation laser interferometry for gravitational wave detection: ACIGA progress, CLASS QUANT, 18(19), 2001, pp. 4121-4126
Reasonable event rate gravitational wave astronomy in the audio frequency d
etection band will require improving the sensitivity of long-baseline inter
ferometer-based gravitational wave detectors currently under construction b
y at least a factor of 10. In this summary we report research being carried
out by the Australian Consortium for Interferometric Gravitational Astrono
my towards this end.