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20242026
most citedStars or gas? Constraining the hardening processes of massive black-hole binaries with LISA

11 citations · 29 across the 10 of their papers we have counts for

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Showing 2025Show all

5 papers · 1 filter

gr-qc2025★ 3 cited

Ab uno disce omnes: Single-harmonic search for extreme mass-ratio inspirals

Lorenzo Speri, Rodrigo Tenorio, Christian Chapman-Bird +1

Extreme mass-ratio inspirals (EMRIs) are one of the key sources of gravitational waves for space-based detectors such as LISA. However, their detection remains a major data analysi…

astro-ph.HE2025★ 5 cited

Where did Heavy Binaries Go? Gravitational-wave Populations Using Delaunay Triangulation with Optimized Complexity

Rodrigo Tenorio, Alexandre Toubiana, Tristan Bruel +2

We investigate the joint mass-redshift evolution of the binary black-hole merger rate in the latest Gravitational-Wave Transient Catalog, GWTC-4.0. We present and apply a novel non…

gr-qc2025★ 2 cited

Comparing astrophysical models to gravitational-wave data in the observable space

Alexandre Toubiana, Davide Gerosa, Matthew Mould +9

Comparing population-synthesis models to the results of hierarchical Bayesian inference in gravitational-wave astronomy requires a careful understanding of the domain of validity o…

astro-ph.GA2025

Bayesian luminosity function estimation in multi-depth datasets with selection effects: A case study for Lyman emitters

Davide Tornotti, Matteo Fossati, Michele Fumagalli +3

We present a hierarchical Bayesian framework designed to infer the luminosity function of any class of object by jointly modelling data from multiple surveys with varying depth, co…

astro-ph.GA2025

A recoiling supermassive black hole in a powerful quasar

Marco Chiaberge, Takahiro Morishita, Matteo Boschini +14

Supermassive black holes (SMBH) are thought to grow through accretion of matter and mergers. Models of SMBH mergers have long suffered the final parsec problem, where SMBH binaries…