Willke, B ; Aufmuth, P ; Aulbert, C ; Babak, S ; Balasubramanian, R ; Barr, B W ; Berukoff, S ; Bose, S ; Cagnoli, G ; Casey, M M ; Churches, D ; Clubley, D ; Colacino, C N ; Crooks, D R M ; Cutler, C ; Danzmann, K ; Davies, R ; Dupuis, R ; Elliffe, E ; Fallnich, C ; Freise, A ; Goßler, S ; Grant, A ; Grote, H ; Heinzel, G ; Heptonstall, A ; Heurs, M ; Hewitson, M ; Hough, J ; Jennrich, O ; Kawabe, K ; Kötter, K ; Leonhardt, V ; Lück, H ; Malec, M ; McNamara, P W ; McIntosh, S A ; Mossavi, K ; Mohanty, S ; Mukherjee, S ; Nagano, S ; Newton, G P ; Owen, B J ; Palmer, D ; Papa, M A ; Plissi, M V ; Quetschke, V ; Robertson, D I ; Robertson, N A ; Rowan, S ; Rüdiger, A ; Sathyaprakash, B S ; Schilling, R ; Schutz, B F ; Senior, R ; Sintes, A M ; Skeldon, K D ; Sneddon, P ; Stief, F ; Strain, K A ; Taylor, I ; Torrie, C I ; Vecchio, A ; Ward, H ; Weiland, U ; Welling, H ; Williams, P ; Winkler, W ; Woan, G ; Zawischa, I (2002) The GEO 600 gravitational wave detector Classical and Quantum Gravity, 19 (7). pp. 1377-1387. ISSN 0264-9381
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Official URL: http://doi.org/10.1088/0264-9381/19/7/321
Related URL: http://dx.doi.org/10.1088/0264-9381/19/7/321
Abstract
The GEO 600 laser interferometer with 600 m armlength is part of a worldwide network of gravitational wave detectors. Due to the use of advanced technologies like multiple pendulum suspensions with a monolithic last stage and signal recycling, the anticipated sensitivity of GEO 600 is close to the initial sensitivity of detectors with several kilometres armlength. This paper describes the subsystems of GEO 600, the status of the detector by September 2001 and the plans towards the first science run.
| Item Type: | Article |
|---|---|
| Source: | Copyright of this article belongs to IOP Publishing. |
| ID Code: | 135593 |
| Deposited On: | 22 Jun 2023 07:28 |
| Last Modified: | 22 Jun 2023 07:28 |
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