Seismic isolation and suspension systems for Advanced LIGO

Norna A. Robertson(California Institute of Technology), R. Mittleman(Massachusetts Institute of Technology), S. Goßler, M. A. Barton(California Institute of Technology), A. Baglino(Stanford University), G. Cagnoli(Université Claude Bernard Lyon 1), Anurag Ganguli(Stanford University), R. X. Adhikari, Claire Campbell(Stanford University), D. C. Coyne(California Institute of Technology), E. J. Daw, Harald Lueck, J. Heefner(California Institute of Technology), J. Hough(University of Glasgow), N. A. Lockerbie(University of Glasgow), Lynne Jones, J. A. Giaime(Louisiana State University), J.‐P. Lacour(Centre Hospitalier Universitaire de Nice), D. Cook(California Institute of Technology), W. Hua(Stanford University), J Faludi(Stanford University), H. Armandula(California Institute of Technology), D. R. M. Crooks(University of Glasgow), B. Lantz(Stanford University), K.A. Lilienkamp(Massachusetts Institute of Technology), C. Hardham(Stanford University), K. Carter(LIGO Scientific Collaboration), J. Greenhalgh(Stanford University), K.O. Mason(Stanford University), J. E. Hanson(LIGO Scientific Collaboration), Jonathan E. Kern(LIGO Scientific Collaboration), Peter Fritschel, Rolf Bork(California Institute of Technology), Gregory M Harry(Stanford University), Alistair Heptonstall(University of Glasgow), A. Grant(University of Glasgow), Daniel B. DeBra(Stanford University), S. M. Aston(University of Birmingham), M. MacInnis(Stanford University), K. Mailand(California Institute of Technology), M. Hammond(LIGO Scientific Collaboration), R. Jones(University of Glasgow), B. Bland, D. Hoyland(University of Birmingham), R. Abbott(National Heart Foundation of Australia), B. P. Abbott(California Institute of Technology), G. Allen(Stanford University), E. J. Elliffe(University of Glasgow), J. Bogenstahl(University of Glasgow), C. A. Cantley(University of Glasgow)
Proceedings of SPIE, the International Society for Optical Engineering/Proceedings of SPIE
September 29, 2004
Cited by 34


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