Stefano Borgani

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Full professor

University of Trieste

Italy

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Stefano Borgani is a Full Professor at the University of Trieste, Italy. His research areas include cosmological simulations, galaxy formation, and the intricate dynamics within galaxy clusters. His recent articles reflect a focus on the interplay between gas and stars, cosmological analysis, and black hole evolution within these frameworks. He is actively involved in projects such as the Three Hundred project and Euclid preparation, contributing significantly to the understanding of the universe's structure and formation.

Recent Grants

Grant: Close

I barioni diffusi nella storia dell'Universo

Open Date: 2008-09-01

Close Date: 2010-08-01

Grant: Close

Observing and modelling the properties of diffuse baryons in clusters of galaxies

Open Date: 2007-04-01

Close Date: 2009-04-01

Stefano Borgani

Research Interests

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Contact this professor

About

Recent Grants

Articles (25)

The Three Hundred project hydrodynamical simulations: Hydrodynamical weak-lensing cluster mass biases and richnesses using different hydro models

Feeding and feedback processes in the Spiderweb proto-intracluster medium (Corrigendum)

The full iron budget in simulated galaxy clusters: The chemistry between gas and stars

DUCA: Dynamic Universe Cosmological Analysis

Galaxy populations of protoclusters in cosmological hydrodynamical simulations

The robustness of cluster clustering covariance calibration

Euclid preparation: XXXIX. The effect of baryons on the halo mass function

Euclid preparation

Euclid preparation

Cosmology with galaxy cluster properties using machine learning

Inferring intrahalo light from stellar kinematics

SubDLe: Identification of substructures in cosmological simulations with deep learning

From Vlasov-Poisson to Schrödinger-Poisson: Dark matter simulation with a quantum variational time evolution algorithm

Cosmological constraints from the abundance, weak lensing, and clustering of galaxy clusters: Application to the SDSS

Feeding and feedback processes in the Spiderweb proto-intracluster medium

Dynamical friction and the evolution of black holes in cosmological simulations: A new implementation in OpenGadget3

Euclid preparation

Intertwined formation of H2, dust, and stars in cosmological simulations

The probability of galaxy–galaxy strong lensing events in hydrodynamical simulations of galaxy clusters

The 700 ks Chandra Spiderweb Field

The Spiderweb Protocluster is Being Magnetized by Its Central Radio Jet

The BEHOMO project: Λ Lemaître-Tolman-Bondi N-body simulations

An excess of small-scale gravitational lenses observed in galaxy clusters

Constraining the origin and models of chemical enrichment in galaxy clusters using the Athena X-IFU

Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time

Collaborators (20)

William GILLARD

Jussi Valiviita

Seshadri Nadathur

Per Lilje

Hannu Kurki-Suonio

Stefano Camera

Elina Keihänen

Martin Kunz

Yannick Copin

Gabriele Mainetti

Konstantinos Tanidis

Alessio Spurio Mancini

Nicola Rosario Napolitano

Massimo Meneghetti

Anastasio Diaz-Sanchez

Eugene Churazov

Pierluigi Monaco

Rafael Toledo-Moreo

Federico Marulli

Chiara SIRIGNANO

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