Isolation from seismic motion is vital for vibration sensitive experiments. The seismic attenuation system (SAS) is a passive mechanical isolation system for optics suspensions. The low natural frequency of a SAS allows seismic isolation starting below 0.2 Hz. The desired isolation at frequencies above a few hertz is 70–80 dB in both horizontal and vertical degrees of freedom. An introduction to the SAS for the AEI 10 m Prototype, an overview of the mechanical design and a description of the major components are given
We present a compact, vacuum compatible seismic attenuation system designed to isolate five auxiliar...
At present a 10\,m prototype interferometer facility is being set up at the AEI Hannover. One unique...
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 ...
Abstract: High precision measurements in various applications rely on active seismic isolation to de...
The 10 m prototype facility at the Albert-Einstein-institute (AEI) in Hanover, Germany, employs thre...
TAMA300 has been upgraded to improve the sensitivity at low frequencies after the last observation r...
The first direct observation of gravitational waves on the 14th September 2015 opened up a new windo...
New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave int...
The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device expressly d...
A new passive seismic attenuation system is being developed to replace the current passive attenuati...
Interferometric Gravitational Wave Detectors, coming online lin late 2000, look for small space stra...
The second/third generation interferometric gravitational wave detectors need not only strong attenu...
In November 2011 a major upgrade of the Virgo gravitational wave detector was started. After these i...
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
We present a compact, vacuum compatible seismic attenuation system designed to isolate five auxiliar...
At present a 10\,m prototype interferometer facility is being set up at the AEI Hannover. One unique...
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 ...
Abstract: High precision measurements in various applications rely on active seismic isolation to de...
The 10 m prototype facility at the Albert-Einstein-institute (AEI) in Hanover, Germany, employs thre...
TAMA300 has been upgraded to improve the sensitivity at low frequencies after the last observation r...
The first direct observation of gravitational waves on the 14th September 2015 opened up a new windo...
New seismic pre-isolation systems will have to be included in the forthcoming gravitational wave int...
The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device expressly d...
A new passive seismic attenuation system is being developed to replace the current passive attenuati...
Interferometric Gravitational Wave Detectors, coming online lin late 2000, look for small space stra...
The second/third generation interferometric gravitational wave detectors need not only strong attenu...
In November 2011 a major upgrade of the Virgo gravitational wave detector was started. After these i...
Abstract. The Horizontal Access Module Seismic Attenuation System (HAM-SAS) is a mechanical device e...
We present a compact, vacuum compatible seismic attenuation system designed to isolate five auxiliar...
At present a 10\,m prototype interferometer facility is being set up at the AEI Hannover. One unique...
Laser interferometric Gravitational Wave telescopes are limited in sensitivity by seismic noise in t...