Abstract The Laser Interferometer Space Antenna (LISA) is the first scientific endeavour to
detect and study gravitational waves from space. LISA will survey the sky for Gravitational …

In a previous article, we have reported on the first subpicometer interferometer flown in
space as part of ESA's LISA Pathfinder mission, and have shown the residual sensor noise …

In the months since the publication of the first results, the noise performance of LISA
Pathfinder has improved because of reduced Brownian noise due to the continued decrease …

Following the selection of The Gravitational Universe by ESA, and the successful flight of
LISA Pathfinder, the LISA Consortium now proposes a 4 year mission in response to ESA's …

We report the first results of the LISA Pathfinder in-flight experiment. The results demonstrate
that two free-falling reference test masses, such as those needed for a space-based …

We present an in-depth analysis of the LISA Pathfinder differential acceleration performance
over the entire course of its science operations, spanning approximately 500 days. We …

We present an optically detected mechanical accelerometer that achieves a sensitivity of
100 ngn/Hz over a bandwidth of 10 kHz and is traceable. We have incorporated a Fabry …

The charge accumulation caused by cosmic rays and solar energetic particles poses a
significant challenge as a source of noise for inertial sensors used in space gravitational …

One of the most common assumptions in the study of neutron star models and their
oscillations is that the pressure is isotopic, however, there are arguments that this may not …

We report the in-orbit operation of a photon-pair source aboard a 1.65-kg nanosatellite and
demonstrate pair generation and polarization correlation under space conditions. The in …