425 citations · 4.2k across the 51 of their papers we have counts for
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Gravitational-wave signal-to-noise interpolation via neural networks
Kaze W. K. Wong, Ken K. Y. Ng, Emanuele Berti
Computing signal-to-noise ratios (SNRs) is one of the most common tasks in gravitational-wave data analysis. While a single SNR evaluation is generally fast, computing SNRs for an…
Astrophysical implications of GW190412 as a remnant of a previous black-hole merger
Davide Gerosa, Salvatore Vitale, Emanuele Berti
Two of the dominant channels to produce merging stellar-mass black-hole binaries are believed to be the isolated evolution of binary stars in the field and dynamical formation in s…
Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations
Margherita Fasano, Kaze W. K. Wong, Andrea Maselli +3
Gravitational waves from the merger of two neutron stars cannot be easily distinguished from those produced by a comparable-mass mixed binary in which one of the companions is a bl…
The mass gap, the spin gap, and the origin of merging binary black holes
Vishal Baibhav, Davide Gerosa, Emanuele Berti +3
Two of the dominant channels to produce the black-hole binary mergers observed by LIGO and Virgo are believed to be the isolated evolution of stellar binaries in the field and dyna…
Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap
Davide Gerosa, Emanuele Berti
Pair instabilities in supernovae might prevent the formation of black holes with masses between and . Multiple generations of black-hole mergers…
Constraining the fraction of binary black holes formed in isolation and young star clusters with gravitational-wave data
Yann Bouffanais, Michela Mapelli, Davide Gerosa +4
Ten binary black-hole mergers have already been detected during the first two observing runs of advanced LIGO and Virgo, and many more are expected to be observed in the near futur…