activity
20242026
most citedIs GN-z11 powered by a super-Eddington massive black hole?

8 citations · 16 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2026

Exploring the observed properties of JWST Little Red Dots with cosmological simulations and dust radiative transfer

Saksham Chandna, Fabio Di Mascia, Simona Gallerani +6

JWST has uncovered compact high-redshift (z>=4) sources, dubbed Little Red Dots (LRDs), characterised by a distinct V-shaped continuum. Their nature remains debated since broad-lin…

astro-ph.GA2026★ 1 cited

Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability

Chaitra, Antonio Ragagnin, Milena Valentini +3

Cosmological hydrodynamical simulations are powerful tools for studying galaxy formation, yet their predictive precision is limited by stochastic variability and numerical uncertai…

astro-ph.GA2025★ 1 cited

Dynamical friction and massive black hole orbits: analytical predictions and numerical solutions

Alice Damiano, Stefano Borgani, Milena Valentini +4

We investigate the orbital decay of a massive BH embedded in a dark matter halo and a stellar bulge, using both analytical and numerical simulations with the aim of developing and…

astro-ph.GA2025★ 3 cited

Simulating nearby disc galaxies on the main star formation sequence II. The gas structure transition in low and high stellar mass discs

Pierrick Verwilghen, Eric Emsellem, Florent Renaud +14

Recent hydrodynamical simulations of isolated barred disc galaxies have suggested a structural change in the distribution of the interstellar medium (ISM) around a stellar mass M$_…

astro-ph.CO2025★ 2 cited

On the Robustness of Cluster Clustering Covariance Calibration

Alessandra Fumagalli, Tiago Castro, Stefano Borgani +1

Ongoing and upcoming wide-field surveys at different wavelengths will measure the distribution of galaxy clusters with unprecedented precision, demanding accurate models for the tw…

astro-ph.GA2025★ 1 cited

Multi-wavelength properties of LISA detectable events

Srija Chakraborty, Simona Gallerani, Fabio Di Mascia +5

We investigate the intrinsic and observational properties of galaxies hosting coalescing massive black holes (MBHs) that gives rise to gravitational waves (GWs) detect…

astro-ph.GA2024★ 8 cited

Is GN-z11 powered by a super-Eddington massive black hole?

Maulik Bhatt, Simona Gallerani, Andrea Ferrara +6

Observations of quasars powered by supermassive black holes (SMBHs; ) challenge our current understanding of early black hole (BH) f…