50 citations · 156 across the 19 of their papers we have counts for
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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…