collaborators

6 papers

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.HE2025

Test for LISA foreground Gaussianity and stationarity: galactic white-dwarf binaries

Riccardo Buscicchio, Antoine Klein, Valeriya Korol +4

Upcoming space-based gravitational-wave detectors will be sensitive to millions and resolve tens of thousands of stellar-mass binary systems at mHz frequencies. The vast majority o…

astro-ph.HE2025

Identifying galactic binary systems of neutron stars and black holes with LISA

Hannah Middleton, Panagiota Kolitsidou, Antoine Klein +3

The Laser Interferometer Space Antenna (LISA) will detect galactic binary systems comprised of black holes and neutron stars. Distinguishing these binaries from the $\si…

astro-ph.IM2025

Bahamas: BAyesian inference with HAmiltonian Montecarlo for Astrophysical Stochastic background

Federico Pozzoli, Riccardo Buscicchio, Antoine Klein +1

The LISA datastream will be populated by large instrumental and astrophysical noises, both potentially exhibiting long-term non-stationarities. Modelling and inferring on them is a…

astro-ph.GA2025

Cyclostationary signals in LISA: a practical application to Milky Way satellites

Federico Pozzoli, Riccardo Buscicchio, Antoine Klein +3

One of the primary sources of gravitational waves (GWs) anticipated to be detected by the Laser Interferometer Space Antenna (LISA) are Galactic double white dwarf binaries (DWDs).…

astro-ph.HE2025

Stars or gas? Constraining the hardening processes of massive black-hole binaries with LISA

Alice Spadaro, Riccardo Buscicchio, David Izquierdo-Villalba +3

Massive black-hole binaries will be the loudest sources detectable by LISA. These systems are predicted to form during the hierarchical assembly of cosmic structures and coalesce b…