Kenneth Strain, B. Allen, P. Aufmuth, C. Aulbert, S. Babak, R. Balasubramanian, B. Barr, S. Berukoff, A. Bunkowski, Gianpietro Cagnoli, C. Cantley, M. Casey, S. Chelkowski, D. Churches, T. Cokelaer, C. Colacino, David Crooks, C. Cutler, Karsten Danzmann, R. Davies, Rejean Dupuis, E. Elliffe, Carsten Fallnich, A. Franzen, A. Freise, S. Gossler, A. Grant, H. Grote, S. Grunewald, J. Harms, Gerhard Heinzel, Ik Heng, A. Hepstonstall, M. Heurs, M. Hewitson, S. Hild, James Hough, Y. Itoh, R. Jones, S. Huttner, K. Kawabe, Christian Killow, K. Koetter, B. Krishnan, V. Leonhardt, Harald Lueck, B. Machenschalk, M. Malec, R. Mercer, Christopher Messenger, S. Mohanty, Kasem Mossavi, S. Mukherjee, P. Murray, S. Nagano, G. Newton, M. Papa, M. Perreur-Lloyd, M. Pitkin, M. Plissi, V. Quetschke, Virginia Re, S. Reid, L. Ribichini, D. Robertson, Norna Robertson, J. Romano, Sheila Rowan, Albrecht Ruediger, Bangalore Sathyaprakash, R. Schilling, R. Schnabel, B. Schutz, F. Seifert, A. Sintes, J. Smith, Peter Sneddon, I. Taylor, R. Taylor, A. Thuering, Carlo Ungarelli, H. Vahlbruch, Alberto Vecchio, J. Veitch, Harry Ward, U. Weiland, Herbert Welling, P. Williams, Benno Willke, Walter Winkler, Graham Woan, Ivo Zawischa
The GEO 600 laser interferometer with 600m armlength is part of a worldwide network of gravitational wave detectors. GEO 600 is unique in having advanced multiple pendulum suspensions with a monolithic last stage and in employing a signal recycled optical design. This paper describes the recent commissioning of the interferometer and its operation in signal recycled mode.
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