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Autor:
B. J. J. Slagmolen, Susan M. Scott, Raymond Burston, Li Ju, Slawomir Gras, G. de Vine, R. Burman, E. Chin, Florin Garoi, Eric Howell, Sascha Schediwy, M Aoun, Malcolm B. Gray, Andrew Woolley, Zewu Yan, Antony C. Searle, C. M. Mow-Lowry, Jesper Munch, K T Lee, John Winterflood, Jerome Degallaix, J. C. Dumas, Chunnong Zhao, Pablo Barriga, D. J. Hosken, J Jacob, B. J. Cusack, Thu-Lan Kelly, X T Chin, C Y Lee, Damien Mudge, David Coward, A. Brooks, B. Lee, David Blair, T Lun, Benjamin Sheard, David E. McClelland, P. J. Veitch
Publikováno v:
Classical and Quantum Gravity. 21:S887-S893
Advanced laser interferometer detectors utilizing more than 100 W of laser power and with ~106 W circulating laser power present many technological problems. The Australian Consortium for Interferometric Gravitational Astronomy (ACIGA) is developing