29 September 2004 The status of GEO 600
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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.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Kenneth A. Strain, Kenneth A. Strain, B. Allen, B. Allen, P. Aufmuth, P. Aufmuth, C. Aulbert, C. Aulbert, S. Babak, S. Babak, R. Balasubramanian, R. Balasubramanian, B. W. Barr, B. W. Barr, S. Berukoff, S. Berukoff, A. Bunkowski, A. Bunkowski, Gianpietro Cagnoli, Gianpietro Cagnoli, C. A. Cantley, C. A. Cantley, M. M. Casey, M. M. Casey, S. Chelkowski, S. Chelkowski, D. Churches, D. Churches, T. Cokelaer, T. Cokelaer, C. N. Colacino, C. N. Colacino, David R.M. Crooks, David R.M. Crooks, C. Cutler, C. Cutler, Karsten Danzmann, Karsten Danzmann, R. Davies, R. Davies, Rejean J. Dupuis, Rejean J. Dupuis, E. Elliffe, E. Elliffe, Carsten Fallnich, Carsten Fallnich, A. Franzen, A. Franzen, A. Freise, A. Freise, S. Gossler, S. Gossler, A. Grant, A. Grant, H. Grote, H. Grote, S. Grunewald, S. Grunewald, J. Harms, J. Harms, Gerhard Heinzel, Gerhard Heinzel, Ik Siong Heng, Ik Siong Heng, A. Hepstonstall, A. Hepstonstall, M. Heurs, M. Heurs, M. Hewitson, M. Hewitson, S. Hild, S. Hild, James Hough, James Hough, Y. Itoh, Y. Itoh, R. Jones, R. Jones, S. H. Huttner, S. H. Huttner, K. Kawabe, K. Kawabe, Christian Killow, Christian Killow, K. Koetter, K. Koetter, B. Krishnan, B. Krishnan, V. Leonhardt, V. Leonhardt, Harald Lueck, Harald Lueck, B. Machenschalk, B. Machenschalk, M. Malec, M. Malec, R. Adam Mercer, R. Adam Mercer, Christopher Messenger, Christopher Messenger, S. Mohanty, S. Mohanty, Kasem Mossavi, Kasem Mossavi, S. Mukherjee, S. Mukherjee, P. Murray, P. Murray, S. Nagano, S. Nagano, G. P. Newton, G. P. Newton, M. A. Papa, M. A. Papa, M. Perreur-Lloyd, M. Perreur-Lloyd, M. Pitkin, M. Pitkin, M. V. Plissi, M. V. Plissi, V. Quetschke, V. Quetschke, Virginia Re, Virginia Re, S. Reid, S. Reid, L. Ribichini, L. Ribichini, D. I. Robertson, D. I. Robertson, Norna A. Robertson, Norna A. Robertson, J. D. Romano, J. D. Romano, Sheila Rowan, Sheila Rowan, Albrecht Ruediger, Albrecht Ruediger, Bangalore S. Sathyaprakash, Bangalore S. Sathyaprakash, R. Schilling, R. Schilling, R. Schnabel, R. Schnabel, B. F. Schutz, B. F. Schutz, F. Seifert, F. Seifert, A. M. Sintes, A. M. Sintes, J. R. Smith, J. R. Smith, Peter H. Sneddon, Peter H. Sneddon, I. Taylor, I. Taylor, R. Taylor, R. Taylor, A. Thuering, A. Thuering, Carlo Ungarelli, Carlo Ungarelli, H. Vahlbruch, H. Vahlbruch, Alberto Vecchio, Alberto Vecchio, J. Veitch, J. Veitch, Harry Ward, Harry Ward, U. Weiland, U. Weiland, Herbert Welling, Herbert Welling, P. Williams, P. Williams, Benno Willke, Benno Willke, Walter Winkler, Walter Winkler, Graham Woan, Graham Woan, Ivo Zawischa, Ivo Zawischa, } "The status of GEO 600", Proc. SPIE 5500, Gravitational Wave and Particle Astrophysics Detectors, (29 September 2004); doi: 10.1117/12.551127; https://doi.org/10.1117/12.551127

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