Abstract
The Japanese gravitational wave detection group plans to build LCGT to establish gravitational wave astronomy, and then launch DECIGO to open a new window of gravitational wave astronomy. We have been working on TAMA300 and CLIO to demonstrate technologies required to build LCGT. We also have been developing DECIGO pathfinder for the first step toward the realization of DECIGO.
© 2009 Optical Society of America
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