We present a novel inertial sensor designed and developed at Nikhef that features an interferometric readout for a horizontal monolithic accelerometer. It is the first time this class of mechanics and this type of optical readout are combined. It will be able to measure 3 × 10-15 m/√HZ displacement levels from 20 Hz onwards. Current results show (self) noise levels of 8×10-15 m/√Hz from 30 Hz onwards. Despite these unprecedented results, the result is worse than the sum of modeled noise contributions. Several possible unmodeled noise sources and possible solutions have been identified
A tunable mechanical horizontal monolithic seismometer-accelerometer, developed for applications in ...
The design and mechanics for a new very-low noise low frequency horizontal accelerometer is presente...
Laser interferometric Gravitational Wave telescopes are limited in sensitivity by seismic noise in t...
We present a novel inertial sensor designed and developed at Nikhef that features an interferometric...
High precision interferometers such as gravitational-wave detectors require complex seismic isolatio...
The European Gravitational wave Observatory Virgo is undergoing an upgrade to increase its strain se...
The European Gravitational wave Observatory Virgo is undergoing an upgrade to increase its strain se...
In order to achieve the excellent seismic isolation necessary for the operation of gravitational wav...
Nowadays, sensors’ resolution limits their performance at low frequency which reduces their operatin...
The readout system of a new very low noise low-frequency, force-feedback accelerometer is presented....
Inertial sensors are devices capable of measuring the absolute motion of the support they are fixed ...
The Virgo Gravitational Wave Observatory (Cascina, Italy) has encountered problems with scat-tered l...
Large-scale, high-end, scientific instruments see their performances significantly impaired by resid...
This paper describes a new implementation of monolithic horizontal sensor, developed at the Universi...
A tunable mechanical horizontal monolithic seismometer-accelerometer, developed for applications in ...
The design and mechanics for a new very-low noise low frequency horizontal accelerometer is presente...
Laser interferometric Gravitational Wave telescopes are limited in sensitivity by seismic noise in t...
We present a novel inertial sensor designed and developed at Nikhef that features an interferometric...
High precision interferometers such as gravitational-wave detectors require complex seismic isolatio...
The European Gravitational wave Observatory Virgo is undergoing an upgrade to increase its strain se...
The European Gravitational wave Observatory Virgo is undergoing an upgrade to increase its strain se...
In order to achieve the excellent seismic isolation necessary for the operation of gravitational wav...
Nowadays, sensors’ resolution limits their performance at low frequency which reduces their operatin...
The readout system of a new very low noise low-frequency, force-feedback accelerometer is presented....
Inertial sensors are devices capable of measuring the absolute motion of the support they are fixed ...
The Virgo Gravitational Wave Observatory (Cascina, Italy) has encountered problems with scat-tered l...
Large-scale, high-end, scientific instruments see their performances significantly impaired by resid...
This paper describes a new implementation of monolithic horizontal sensor, developed at the Universi...
A tunable mechanical horizontal monolithic seismometer-accelerometer, developed for applications in ...
The design and mechanics for a new very-low noise low frequency horizontal accelerometer is presente...
Laser interferometric Gravitational Wave telescopes are limited in sensitivity by seismic noise in t...