6 citations · 7 across the 4 of their papers we have counts for
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astro-ph.GA2026
Isolated or Dynamical? Tracing Black Hole Binary Formation through the Population of Gravitational-Wave Sources
Manuel Arca Sedda, Lavinia Paiella, Cristiano Ugolini +5
The population of binary black hole (BBH) mergers observed by the LIGO-Virgo-KAGRA (LVK) collaboration offers a window into the cosmic evolution of compact binaries and their forma…
astro-ph.GA2025★ 6 cited
Seeds to success: growing heavy black holes in dense star clusters
Lavinia Paiella, Manuel Arca Sedda, Benedetta Mestichelli +1
The observational dearth of black holes (BHs) with masses between 100 and 100,000 raises questions about the nature of intermediate-mass black holes (IMBHs). Propos…
astro-ph.GA2025★ 1 cited
The assembly of intermediate black holes with complementary approaches: Dragon II and BPop
Cristiano Ugolini
Intermediate-mass black holes (IMBHs) occupy the range, but their existence remains poorly constrained. Only a few candidates have been suggested in dwarf…