most citedDetectability of Gravitational-Wave Memory with LISA: A Bayesian Approach

3 citations · 3 across the 5 of their papers we have counts for

collaborators

6 papers

gr-qc2026

The Doppler boosted LISA response to gravitational waves

Tom van der Steen, Henri Inchauspé, Thomas Hertog +1

Future space-based gravitational wave observatories like LISA, TianQin and Taji are expected to detect massive black hole binaries (MBHBs) with high signal-to-noise ratios (SNRs),…

gr-qc20263 cited

Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach

Adrien Cogez, Silvia Gasparotto, Jann Zosso +5

Gravitational wave (GW) astronomy opens a new venue to explore the universe. Future observatories such as LISA, the Laser Interferometer Space Antenna, are expected to observe prev…

gr-qc2026

Relativistic signatures of scalar dark matter in extreme-mass-ratio inspirals

Robrecht Keijzer, Simon Maenaut, Henri Inchauspé +1

We study gravitational wave emission by circular extreme-mass-ratio systems in a spherically symmetric scalar environment. Previous studies have focused on the impact of scalar rad…

gr-qc2026

Toward claiming a detection of gravitational memory

Jann Zosso, Lorena Magaña Zertuche, Silvia Gasparotto +3

Gravitational memory is a zero-frequency effect associated with a permanent change in the asymptotic spacetime metric induced by radiation. Although its universal manifestation is…

astro-ph.IM2026

LISA science ground segment conventions

Quentin Baghi, Stanislas Babak, Leor Barack +22

This document sets out the conventions used for data simulations, waveforms, and analysis pipelines within the Distributed Data Processing Centre (DDPC) of the Laser Interferometer…

astro-ph.IM2026

LISA Non-Linear Dynamics and Tilt-To-Length Coupling

Lavinia Heisenberg, Henri Inchauspé, Sarah Paczkowski +1

For the LISA mission, Tilt-To-Length (TTL) coupling is expected to be one of the dominant instrumental noise contributions after laser frequency noise is suppressed based, on assum…