11 citations · 29 across the 10 of their papers we have counts for
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Inferring the population properties of galactic binaries from LISA's stochastic foreground
Federico De Santi, Alessandro Santini, Alexandre Toubiana +2
Galactic binaries are expected to be the most numerous LISA sources and to produce a stochastic gravitational-wave foreground whose spectral shape encodes information about the und…
Exceptionality of exceptional gravitational-wave events
Rodrigo Tenorio, Davide Gerosa
In gravitational-wave astronomy, as in other scientific disciplines, ``exceptional'' sources attract considerable interest because they challenge our current understanding of the u…
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…
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…
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…