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The Center for Gravitational Wave Astronomy (CGWA) is funded by NASA and will focus on three major research areas: gravitational wave data analysis, gravitational wave source modeling, and phenomenological astrophysics of supermassive black holes. The proposed research is relevant to the NASA Space Science Enterprise of charting the evolution of the universe and understanding its galaxies, stars, and their dynamics and evolution. In particular, we expect the center to make important contributions to LISA (Laser Interferometric Space Antenna), a joint NASA-ESA mission with a projected launch date of 2011. LISA consists of three identical spacecraft located in an equilateral triangle km on a side in a heliocentric orbit. The spacecraft carry the optical components of a Michelson-Morley interferometer, which will measure the passing of gravitational waves of astrophysical origin in the to Hz band. NASA's recognition of the technological and scientific opportunities presented by the LISA mission is exemplified in their selection of the Disturbance Reduction System technology as the Space Technology 7 project for the New Millennium Program.



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