55 citations · 534 across the 23 of their papers we have counts for
23 papers
Galaxy populations of ProtoClusters in cosmological hydrodynamical simulations
Michela Esposito, Stefano Borgani, Veronica Strazzullo +6
The study of protoclusters at cosmic noon is essential to understand the impact on galaxies of the environment and of the transformational processes occurring in this epoch. This w…
Intertwined Formation of , Dust, and Stars in Cosmological Simulations
Cinthia Ragone-Figueroa, Gian Luigi Granato, Massimiliano Parente +4
Context: Molecular hydrogen () is crucial in galaxy formation and evolution, serving as the main fuel for star formation (SF). In metal-enriched environments, …
Probing massive black holes with gravitational waves
Srija Chakraborty, Simona Gallerani, Tommaso Zana +6
We investigate the coalescence of massive black hole () binaries (MBHBs) at by adopting a suite of cosmological hydrodynamical simu…
Simulating the LOcal Web (SLOW): I. Anomalies in the local density field
Klaus Dolag, Jenny G. Sorce, Sergey Pilipenko +5
Context: Several observations of the local Universe (LU) point towards the existence of very prominent structures. The presence of massive galaxy clusters and local super clusters…
The Cosmological Simulation Code OpenGadget3 -- Implementation of Meshless Finite Mass
Frederick Groth, Ulrich P. Steinwandel, Milena Valentini +1
Subsonic turbulence plays a major role in determining properties of the intra cluster medium (ICM). We introduce a new Meshless Finite Mass (MFM) implementation in OpenGadget3 and…
Is the star formation rate in quasars overestimated?
Fabio Di Mascia, Stefano Carniani, Simona Gallerani +4
The large total infrared (TIR) luminosities () observed in quasars are generally converted into high star formation rates ($SFR \gtr…