A report on the status of the GEO 600 gravitational wave detector, M Hewitson, P Aufmuth, C Aulbert, S Babak, R Balasubramanian, B W Barr, S Berukoff, G Cagnoli, C A Cantley, M M Casey, S Chelkowski, D Churches, C N Colacino, D R M Crooks, C Cutler, K Danzmann, R Davies, R Dupuis, E Elliffe, C Fallnich, A Freise, S Goßler, A Grant, H Grote, S Grunewald, J Harms, G Heinzel, S Heng, A Hepstonstall, M Heurs, J Hough, Y Itoh, O Jennrich, R Jones, S Hutter, K Kawabe, C Killow, K Kötter, B Krishnan, V Leonhardt, H Lück, B Machenschalk, M Malec, K Mossavi, S Mohanty, S Mukherjee, S Nagano, G P Newton, M A Papa, M Perreur-Lloyd, M Pitkin, M V Plissi, V Quetschke, S Reid, L Ribichini, D I Robertson, N A Robertson, S Rowan, A Rüdiger, B S Sathyaprakash, R Schilling, R Schnabel, B F Schutz, F Seifert, A M Sintes, J Smith, P Sneddon, K A Strain, I Taylor, C I Torrie, A Vecchio, H Ward, U Weiland, H Welling, P Williams, B Willke, W Winkler, G Woan, I Zawischa
No takes yet. Share an insight, caveat, or question.
Hewitson et al. (2003) studied this question.