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All the large interferometric gravitational wave detectors use power recycling in order to enhance the circulating light power. In GEO600 an advanced optical layout is used including a novel design of suspensions for reducing thermal noise effects and including signal recycling, a resonant enhancement of periodic signals. Several technical problems had to be solved since the installation of the signal-recycling mirror in late 2002, but now stable operation with lock stretches of days has been demonstrated. So GEO600 is the first long-baseline gravitational wave detector in the dual-recycling configuration.
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