collaborators

5 papers

astro-ph.CO2026

Exploring future synergies for large-scale structure between gravitational waves and radio sources

Stefano Zazzera, José Fonseca, Tessa Baker +1

Future third-generation gravitational wave detectors like the Einstein Telescope (ET) and Cosmic Explorer (CE) are expected to detect millions of binary black hole (BBH) mergers. A…

astro-ph.CO2026

Large scale structure prior knowledge in the dark siren method

Charles Dalang, Bartolomeo Fiorini, Tessa Baker

Gravitational wave dark sirens are a powerful tool for cosmology and inference of compact object population hyperparameters. They allow for a measurement of the luminosity distance…

astro-ph.CO2026

Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology

Konstantin Leyde, Tessa Baker, Wolfgang Enzi

The dark siren method exploits the complementarity between gravitational-wave binary coalescence signals and galaxy catalogs originating from the same regions of space. However, al…

astro-ph.CO2024

Cosmic Cartography: Bayesian reconstruction of the galaxy density informed by large-scale structure

Konstantin Leyde, Tessa Baker, Wolfgang Enzi

The dark sirens method combines gravitational waves and catalogs of galaxies to constrain the cosmological expansion history, merger rates and mass distributions of compact objects…

astro-ph.CO2024

Gravitational waves and galaxies cross-correlations: a forecast on GW biases for future detectors

Stefano Zazzera, José Fonseca, Tessa Baker +1

Gravitational waves (GWs) have rapidly become important cosmological probes since their first detection in 2015. As the number of detected events continues to rise, upcoming instru…