The upgrade of GEO600
arXiv:1004.0339 · doi:10.1088/1742-6596/228/1/012012
Abstract
The German / British gravitational wave detector GEO 600 is in the process of being upgraded. The upgrading process of GEO 600, called GEO-HF, will concentrate on the improvement of the sensitivity for high frequency signals and the demonstration of advanced technologies. In the years 2009 to 2011 the detector will undergo a series of upgrade steps, which are described in this paper.
9 pages, Amaldi 8 conference contribution
References in corpus (5)
- Titania-doped tantala/silica coatings for gravitational-wave detection
- The path to the enhanced and advanced LIGO gravitational-wave detectors
- Experimental characterization of frequency dependent squeezed light
- DC-readout of a signal-recycled gravitational wave detector
- Broadband squeezing of quantum noise in a Michelson interferometer with Twin-Signal-Recycling
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