1.
Phys Rev Lett
; 86(18): 3950-4, 2001 Apr 30.
Artigo
em Inglês
| MEDLINE
| ID: mdl-11328068
RESUMO
TAMA300, an interferometric gravitational-wave detector with 300-m baseline length, has been developed and operated with sufficient sensitivity to detect gravitational-wave events within our galaxy and sufficient stability for observations; the interferometer was operated for over 10 hours stably and continuously. With a strain-equivalent noise level of h approximately 5x10(-21)/sqrt[Hz], a signal-to-noise ratio of 30 is expected for gravitational waves generated by a coalescence of 1.4M-1.4M binary neutron stars at 10 kpc distance. We evaluated the stability of the detector sensitivity with a 2-week data-taking run, collecting 160 hours of data to be analyzed in the search for gravitational waves.
Assuntos
Astronomia/métodos , Gravitação , Astronomia/instrumentação , Lasers , Sensibilidade e Especificidade
2.
J Electron Microsc (Tokyo)
; 28(1): 49-50, 1979.
Artigo
em Inglês
| MEDLINE
| ID: mdl-469451
3.
Shigaku
; 66(4): 548-53, 1978 Dec.
Artigo
em Japonês
| MEDLINE
| ID: mdl-296332
4.
Shigaku
; 66(1): 117-24, 1978 Jun.
Artigo
em Japonês
| MEDLINE
| ID: mdl-397430
5.
Shigaku
; 65(2): 263-7, 1977 Aug.
Artigo
em Japonês
| MEDLINE
| ID: mdl-275737
6.
Shigaku
; 65(2): 268-82, 1977 Aug.
Artigo
em Japonês
| MEDLINE
| ID: mdl-275738
7.
Shigaku
; 64(2): 332-6, 1976 Aug.
Artigo
em Japonês
| MEDLINE
| ID: mdl-1075437
8.
Nihon Koku Geka Gakkai Zasshi
; 20(6): 659-61, 1974.
Artigo
em Japonês
| MEDLINE
| ID: mdl-4535482