Surf these sites: ACIGA -- The Australian Consortium for Interferometric Gravitational Astronomy. AURIGA -- Ultracryogenic gravitational wave detector experiment at Legnaro National Laboratories, Italy. Australian International Gravitational Research Center -- Gravity wave group at University of Western Australia. Chilling Mirrors with Light -- Applied to gravitational wave detectors. GEO 600 -- A UK-German project aiming at the direct detection of gravitational waves by means of a laser interferometer of 600 m armlength. Gravity Wave Analysis From LIGO Prototype -- Physics News Update. ICRR Group -- Gravitational wave group in Japan. LIGO Home Page -- The Laser Interferometer Gravitational-Wave Observatory (LIGO) project is a pioneering effort to design and construct a novel scientific facility - a gravitational-wave observatory - that will open a new observational window on the universe. Laser Interferometer Space Antenna (LISA) -- An ESA space mission to detect and observe gravitational waves from massive black holes and galactic binary stars in the frequency range 10-4 to 10-1 hz. Useful measurements in this frequency range cannot be made on the ground because of the unshieldable background of local gravitational noise. Laser Interferometer Space Antenna -- LISA -- Project that will attempt to detect gravitational waves. Homepage at NASA. Laser Interferometer Space Antenna -- LISA -- Homepage at the Universität Hannover. Listen to the Universe -- Simulated sounds of gravitational waves created by spiraling binary systems. NAUTILUS -- Gravitational wave antenna, 2300 kg aluminum cylinder cooled to a temperature of 0.1 K. NAUTILUS Observed Cosmic Rays -- Physics News Update. Ripples in Curvature -- Transparencies of a talk by Patrick Brady, included are sound files of compact coalescing binaries. Rome Group -- Rome Gravitational Wave Experiment. TAMA -- A five-year (1995-2000) project involving almost all gravity physics researchers in Japan. It adopts a Fabry-Perot Michelson Interferometer (FPMI) with recycling. The aim of this project is to develop advanced techniques needed for a future km-sized interferometer and catch gravitational waves that may occur by chance within our local group of galaxies. The Virgo Project -- Collaboration between Italian and French research teams for the realization of an interferometric gravitational wave detector. Tsubono group -- 300-m arm-length Fabry-Perot laser interferometer. WUGRAV Movies -- Computer simulated movies of colliding neutron stars, gravitational waves propagation; click on top image for newest movies. Washington University Gravity Group -- WUGRAV, contains large collection of gravity links.
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