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By K Kuroda et al. (Including Hiroyuki Nakano)
Published in Classical and Quantum Gravity 27, 084004 (Monday, April 5, 2010)

Abstract

LCGT shall be planned to be the first-generation detector with an advanced technique for employing a cryogenic mirror in order to firstly detect a gravitational wave, and after detection, the detector will serve as an astronomical tool to observe the Universe through gravitational wave radiation. In collaborative observation with the LIGO, GEO and Virgo projects, LCGT desires to contribute to the enterprise of detecting gravitational wave events by earlier funding. This paper summarizes the LCGT project.