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20022026
most citedChemical enrichment in cosmological, smoothed particle hydrodynamics simulations

687 citations · 5.7k across the 78 of their papers we have counts for

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25 papers · 1 filter

astro-ph.CO2026

Dianoga simulations of galaxy clusters and groups: Properties of the baryonic components

Stefano Borgani, Alice Damiano, Elena Rasia +12

We introduce the Dianoga set of cosmological simulations of galaxy clusters and groups, specifically aimed at studying the impact of the implementation of AGN feedback and star for…

astro-ph.CO2025★ 5 cited

Euclid preparation. Simulating thousands of Euclid spectroscopic skies

Euclid Collaboration, P. Monaco, G. Parimbelli +303

We present two extensive sets of 3500+1000 simulations of dark matter haloes on the past light cone, and two corresponding sets of simulated (`mock') galaxy catalogues that represe…

astro-ph.CO2025

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

Veronica Biffi, Elena Rasia, Stefano Borgani +5

Heavy chemical elements such as iron in the intra-cluster medium (ICM) of galaxy clusters are a signpost of the interaction between the gas and stellar components. Observations of…

astro-ph.CO2024★ 16 cited

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

Alice Damiano, Milena Valentini, Stefano Borgani +5

We implement a sub-resolution prescription for the unresolved dynamical friction onto black holes (BHs) in the OpenGadget3 code. We carry out cosmological simulations of a volume o…

astro-ph.CO2023★ 4 cited

GrGadget: an N-body TreePM relativistic code for cosmological simulations

Eduardo Quintana-Miranda, Pierluigi Monaco, Luca Tornatore

We present the merging of the Particle-Mesh (PM) relativistic Gevolution code with the TreePM Gadget-4 code, with the aim of studying general relativity effects in cosmology. Our c…

astro-ph.CO2022

Galaxies in the central regions of simulated galaxy clusters

Antonio Ragagnin, Massimo Meneghetti, Luigi Bassini +20

In this paper, we assess the impact of numerical resolution and of the implementation of energy input from AGN feedback models on the inner structure of cluster sub-haloes in hydro…

astro-ph.CO2022★ 41 cited

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

Massimo Meneghetti, Antonio Ragagnin, Stefano Borgani +27

Meneghetti et al. (2020) recently reported an excess of galaxy-galaxy strong lensing (GGSL) in galaxy clusters compared to expectations from the LCDM cosmological model. Theoretica…

astro-ph.CO2020★ 9 cited

On the phase-space structure of galaxy clusters from cosmological simulations

I. Marini, A. Saro, S. Borgani +8

Cosmological N-body simulations represent an excellent tool to study the formation and evolution of dark matter (DM) halos and the mechanisms that have originated the universal pro…

astro-ph.CO2018★ 39 cited

Athena X-IFU synthetic observations of galaxy clusters to probe the chemical enrichment of the Universe

E. Cucchetti, E. Pointecouteau, P. Peille +14

Answers to the metal production of the Universe can be found in galaxy clusters, notably within their Intra-Cluster Medium (ICM). The X-ray Integral Field Unit (X-IFU) on board the…

astro-ph.CO2017★ 97 cited

The history of chemical enrichment in the intracluster medium from cosmological simulations

V. Biffi, S. Planelles, S. Borgani +8

The distribution of metals in the intracluster medium (ICM) of galaxy clusters provides valuable information on their formation and evolution, on the connection with the cosmic sta…

astro-ph.CO2014★ 32 cited

Simulated star formation rate functions at z~4-7, and the role of feedback in high-z galaxies

Edoardo Tescari, Antonios Katsianis, Stuart Wyithe +5

We study the role of feedback from supernovae and black holes in the evolution of the star formation rate function (SFRF) of z~4-7 galaxies. We use a new set of cosmological hydrod…

astro-ph.CO2012★ 50 cited

Galactic Winds in Cosmological Simulations of the Circumgalactic Medium

Paramita Barai, Matteo Viel, Stefano Borgani +7

(Abridged) We explore new observationally-constrained sub-resolution models of galactic outflows and investigate their impact on the circumgalactic medium (CGM) over redshifts z =…

astro-ph.CO2012★ 168 cited

Baryon Census in Hydrodynamical Simulations of Galaxy Clusters

Susana Planelles, Stefano Borgani, Klaus Dolag +4

We carry out an analysis of a set of cosmological SPH hydrodynamical simulations of galaxy clusters and groups aimed at studying the total baryon budget in clusters, and how this b…

astro-ph.CO2012★ 32 cited

How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters

Madhura Killedar, Stefano Borgani, Massimo Meneghetti +3

The observed abundance of giant arcs produced by galaxy cluster lenses and the measured Einstein radii have presented a source of tension for LCDM. Previous cosmological tests for…

astro-ph.CO2012★ 29 cited

Tomographic weak lensing shear spectra from large N-body and hydrodynamical simulations

Luciano Casarini, Silvio A. Bonometto, Stefano Borgani +5

Forthcoming experiments will enable us to determine tomographic shear spectra at a high precision level. Most predictions about them have until now been biased on algorithms yieldi…

astro-ph.CO2012★ 237 cited

Lensing and X-ray mass estimates of clusters (SIMULATION)

E. Rasia, M. Meneghetti, R. Martino +10

[Abridged] We present a comparison between weak-lensing (WL) and X-ray mass estimates of a sample of numerically simulated clusters. The sample consists on the 20 most massive obje…

astro-ph.CO2011★ 113 cited

The effects of baryons on the halo mass function

Weiguang Cui, Stefano Borgani, Klaus Dolag +2

We present an analysis of the effects of baryon physics on the halo mass function. The analysis is based on simulations of a cosmological volume. Besides a Dark Matter (DM) only si…

astro-ph.CO2011★ 105 cited

X-ray mass proxies from hydrodynamic simulations of galaxy clusters (paper I)

D. Fabjan, S. Borgani, E. Rasia +4

We present a detailed study of scaling relations between total cluster mass and three mass proxies based on X-ray observables: temperature of the intra-cluster medium, gas mass and…

astro-ph.CO2010★ 49 cited

Cosmic evolution of the CIV in high-resolution hydrodynamic simulations

E. Tescari, M. Viel, V. D'Odorico +4

We investigate the properties of triply ionized Carbon (CIV) in the Intergalactic Medium using a set of high-resolution and large box-size cosmological hydrodynamic simulations of…

astro-ph.CO2010★ 196 cited

The transition from population III to population II-I star formation

U. Maio, B. Ciardi, K. Dolag +2

We present results from the first cosmological simulations which study the onset of primordial, metal-free (population III), cosmic star formation and the transition to the present…

astro-ph.CO2009★ 284 cited

Simulating the effect of AGN feedback on the metal enrichment of galaxy clusters

D. Fabjan, S. Borgani, L. Tornatore +3

We present a study of the effect of AGN feedback on metal enrichment and thermal properties of the intracluster medium (ICM) in hydrodynamical simulations. The cosmological simulat…

astro-ph.CO2009★ 69 cited

Lyman Alpha Emitter Evolution in the Reionization Epoch

P. Dayal, A. Ferrara, A. Saro +3

Combining cosmological SPH simulations with a previously developed Lyman Alpha production/transmission model and the Early Reionization Model (ERM, reionization ends at redshift z~…

astro-ph.CO2009★ 42 cited

The onset of star formation in primordial haloes

Umberto Maio, Benedetta Ciardi, Naoki Yoshida +2

Star formation remains an unsolved problem in astrophysics. Numerical studies of large-scale structure simulations cannot resolve the whole process and their approach usually assum…

astro-ph.CO2009★ 81 cited

Damped Lyman-alpha systems in high-resolution hydrodynamical simulations

Edoardo Tescari, Matteo Viel, Luca Tornatore +1

We investigate the properties of Damped Lyman-alpha systems (DLAs) using high-resolution and large box-size cosmological hydrodynamical simulations of a LambdaCDM model. The numeri…