Stable operation of a 300-m laser interferometer with sufficient sensitivity to detect gravitational-wave events within our galaxy.
Ando M, Arai K, Takahashi R, Heinzel G, Kawamura S, Tatsumi D, Kanda N, Tagoshi H, Araya A, Asada H, Aso Y, Barton MA, Fujimoto MK, Fukushima M, Futamase T, Hayama K, Horikoshi G, Ishizuka H, Kamikubota N, Kawabe K, Kawashima N, Kobayashi Y, Kojima Y, Kondo K, Kozai Y, Kuroda K, Matsuda N, Mio N, Miura K, Miyakawa O, Miyama SM, Miyoki S, Moriwaki S, Musha M, Nagano S, Nakagawa K, Nakamura T, Nakao K, Numata K, Ogawa Y, Ohashi M, Ohishi N, Okutomi S, Oohara K, Otsuka S, Saito Y, Sasaki M, Sato S, Sekiya A, Shibata M, Somiya K, Suzuki T, Takamori A, Tanaka T, Taniguchi S, Telada S, Tochikubo K, Tomaru T, Tsubono K, Tsuda N, Uchiyama T, Ueda A, Ueda K, Waseda K, Watanabe Y, Yakura H, Yamamoto K, Yamazaki T; TAMA Collaboration.
Ando M, et al. Among authors: kawamura s.
Phys Rev Lett. 2001 Apr 30;86(18):3950-4. doi: 10.1103/PhysRevLett.86.3950.
Phys Rev Lett. 2001.
PMID: 11328068
Free article.
