50 citations · 156 across the 19 of their papers we have counts for
20 papers
Population-level correlations in Bayesian statistics: an illustrative model for gravitational-wave astronomy
Caroline B. Owen, Alexandre Toubiana, Davide Gerosa
With increasingly large numbers of gravitational-wave events, population inference is now beginning to move beyond predictions of marginal distributions and to probe correlations b…
Targeting black holes from metal-poor progenitors with next-generation gravitational-wave detectors
Federico Leto di Priolo, Martyna Chruślińska, Davide Gerosa
Next-generation gravitational-wave detectors such as the Einstein Telescope and Cosmic Explorer will be able to detect binary black-hole mergers out to the cosmic dawn. Mergers obs…
Gravitational-wave astronomy requires population-informed parameter estimation
Matthew Mould, Rodrigo Tenorio, Davide Gerosa
Gravitational-wave events are interpreted in terms of Bayesian posteriors for their source properties inferred under unphysical reference priors. Though these parameter estimates a…
Accurate and efficient simulation-based inference for massive black-hole binaries with LISA
Alice Spadaro, Jonathan Gair, Davide Gerosa +7
We develop an accurate simulation-based inference framework for high-mass () black-hole binaries observable by LISA. The method is implemented within th…
Variance of gravitational-wave populations
Alessia Corelli, Davide Gerosa, Matthew Mould +1
We quantify the impact of finite catalog size, or "catalog variance," on current gravitational-wave population analyses. The distribution of merging binary black holes is commonly…
Black-hole ringdown with templates capturing spin precession: A reanalysis of GW190521
Chiara Anselmo, Costantino Pacilio, Davide Gerosa
The ringdown stage of a binary black-hole merger provides a clean probe of strong-field gravity, as it can be modeled with minimal assumptions. The quasi-normal-mode frequencies en…
Impact of facility timing and coordination for next-generation gravitational-wave detectors
Ssohrab Borhanian, Arianna Renzini, Philippa S. Cole +3
While the Einstein Telescope and Cosmic Explorer proposals for next-generation, ground-based detectors promise vastly improved sensitivities to gravitational-wave signals, only joi…
Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
G. Giarda, A. I. Renzini, C. Pacilio +1
Third-generation ground-based gravitational wave detectors are expected to observe of overlapping signals per year from a multitude of astrophysical sources tha…
Sequential simulation-based inference for extreme mass ratio inspirals
Philippa S. Cole, James Alvey, Lorenzo Speri +4
Extreme mass-ratio inspirals pose a difficult challenge in terms of both search and parameter estimation for upcoming space-based gravitational-wave detectors such as LISA. Their s…
Ringdown mode amplitudes of precessing binary black holes
Francesco Nobili, Swetha Bhagwat, Costantino Pacilio +1
The ringdown phase of a binary black-hole merger encodes key information about the remnant properties and provides a direct probe of the strong-field regime of General Relativity.…
Fusing Bluetooth With Pedestrian Dead Reckoning: A Floor Plan-Assisted Positioning Approach
Wenxuan Pan, Yang Yang, Mingzhe Chen +3
Floor plans can provide valuable prior information that helps enhance the accuracy of indoor positioning systems. However, existing research typically faces challenges in efficient…
Sampling the full hierarchical population posterior distribution in gravitational-wave astronomy
Michele Mancarella, Davide Gerosa
We present a full sampling of the hierarchical population posterior distribution of merging black holes using current gravitational-wave data. We directly tackle the most relevant…
Reconstructing parametric gravitational-wave population fits from non-parametric results without refitting the data
Cecilia Maria Fabbri, Davide Gerosa, Alessandro Santini +3
Combining multiple events into population analyses is a cornerstone of gravitational-wave astronomy. A critical component of such studies is the assumed population model, which can…
Forecasting the population properties of merging black holes
Viola De Renzis, Francesco Iacovelli, Davide Gerosa +2
Third-generation gravitational-wave detectors will observe up to millions of merging binary black holes. With such a vast dataset, stacking events into population analyses will arg…
Which is which? Identification of the two compact objects in gravitational-wave binaries
Davide Gerosa, Viola De Renzis, Federica Tettoni +3
Compact objects observed in gravitational-wave astronomy so far always come in pairs and never individually. Identifying the two components of a binary system is a delicate operati…
Flexible mapping of ringdown amplitudes for nonprecessing binary black holes
Costantino Pacilio, Swetha Bhagwat, Francesco Nobili +1
The remnant black hole from a binary coalescence emits ringdown gravitational waves characterized by quasinormal modes, which depend solely on the remnant's mass and spin. In contr…
Quick recipes for gravitational-wave selection effects
Davide Gerosa, Malvina Bellotti
Accurate modeling of selection effects is a key ingredient to the success of gravitational-wave astronomy. The detection probability plays a crucial role in both statistical popula…
Classifying binary black holes from Population III stars with the Einstein Telescope: A machine-learning approach
Filippo Santoliquido, Ulyana Dupletsa, Jacopo Tissino +7
Third-generation (3G) gravitational-wave detectors such as the Einstein Telescope (ET) will observe binary black hole (BBH) mergers at redshifts up to . However, an uneq…
Catalog variance of testing general relativity with gravitational-wave data
Costantino Pacilio, Davide Gerosa, Swetha Bhagwat
Combining multiple gravitational-wave observations allows for stringent tests of general relativity, targeting effects that would otherwise be undetectable using single-event analy…
Numerical simulations of stellar collapse in scalar-tensor theories of gravity
Davide Gerosa, Ulrich Sperhake, Christian D. Ott
We present numerical-relativity simulations of spherically symmetric core collapse and compact-object formation in scalar-tensor theories of gravity. The additional scalar degree o…