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We started improvements of the detector and developments of observation technique in 1995 using the 300m interferometer gravitational antenna TAMA300. In Mitaka campus of the national astronomical observatory of Japan. The aim of the project is to develop advanced techniques needed for a future km-sized interferometer and catch gravitational waves that may occur within our local group of galaxies. The present sensitivity of TAMA300.
Fear is the lock, and laughter the key to your heart. Sorry guys, but this journal is. The Littlest Samurai - A Mijumaru Collection! Powered by LiveJournal.