Add to ORKGTAMA300 has been upgraded to improve the sensitivity at low frequencies after the last observation run in 2004. To avoid the noise caused by seismic activities, we installed a new seismic isolation system —- the TAMA seismic attenuation system (SAS). Four SAS towers for the test-mass mirrors were sequentially installed from 2005 to 2006. The recycled Fabry–Perot Michelson interferometer was successfully locked with the SAS. We confirmed the reduction of both length and angular fluctuations at frequencies higher than 1 Hz owing to the SAS
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
International audienceThe Virgo experiment, located near Pisa, Italy, is a large laser Michelson int...
Laser interferometric Gravitational Wave telescopes are limited in sensitivity by seismic noise in t...
Isolation from seismic motion is vital for vibration sensitive experiments. The seismic attenuation ...
A new seismic isolation system, TAMA Seismic Attenuation System (TAMA-SAS), was installed to TAMA300...
The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device expressly d...
New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave int...
A new passive seismic attenuation system is being developed to replace the current passive attenuati...
In November 2011 a major upgrade of the Virgo gravitational wave detector was started. After these i...
The second/third generation interferometric gravitational wave detectors need not only strong attenu...
The current status of the TAMA and CLIO detectors in Japan is reported in this paper. These two inte...
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
International audienceThe Virgo experiment, located near Pisa, Italy, is a large laser Michelson int...
Laser interferometric Gravitational Wave telescopes are limited in sensitivity by seismic noise in t...
Isolation from seismic motion is vital for vibration sensitive experiments. The seismic attenuation ...
A new seismic isolation system, TAMA Seismic Attenuation System (TAMA-SAS), was installed to TAMA300...
The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device expressly d...
New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave int...
A new passive seismic attenuation system is being developed to replace the current passive attenuati...
In November 2011 a major upgrade of the Virgo gravitational wave detector was started. After these i...
The second/third generation interferometric gravitational wave detectors need not only strong attenu...
The current status of the TAMA and CLIO detectors in Japan is reported in this paper. These two inte...
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
International audienceThe Virgo experiment, located near Pisa, Italy, is a large laser Michelson int...
Laser interferometric Gravitational Wave telescopes are limited in sensitivity by seismic noise in t...