activity
19932026
most citedCosmology and Fundamental Physics with the Euclid Satellite

1k citations · 2.8k across the 17 of their papers we have counts for

collaborators

18 papers

astro-ph.IM2026

The OpenGadget3 Code for Cosmological Simulations

Klaus Dolag, Geray S. Karademir, Luca Tornatore +28

We present the public release of OpenGadget3 (OG3), a substantially extended and re-organised version of the widely used Gadget-2/3 family of cosmological simulation codes. Since G…

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.CO2017★ 2 cited

CLASH-VLT: constraints on gravity models with galaxy clusters using lensing and kinematic analyses

L. Pizzuti, B. Sartoris, L. Amendola +10

We perform a maximum likelihood kinematic analysis of the two dynamically relaxed galaxy clusters MACS J1206.2-0847 at and RXC J2248.7-4431 at to determine the to…

astro-ph.CO2016★ 1k cited

Cosmology and Fundamental Physics with the Euclid Satellite

Luca Amendola, Stephen Appleby, Anastasios Avgoustidis +69

Euclid is a European Space Agency medium class mission selected for launch in 2020 within the Cosmic Vision 2015 2025 program. The main goal of Euclid is to understand the origin o…

astro-ph.GA2015★ 38 cited

Semi-Analytic Model Predictions of the Galaxy Population in Proto-clusters

E. Contini, G. De Lucia, N. Hatch +2

We investigate the galaxy population in simulated proto-cluster regions using a semi-analytic model of galaxy formation, coupled to merger trees extracted from N-body simulations.…

astro-ph.CO2014★ 1 cited

Galaxy Cluster Science with the Sunyaev-Zel'dovich Effect

Keith Grainge, Stefano Borgani, Sergio Colafrancesco +5

Studying galaxy clusters through their Sunyaev-Zel'dovich (SZ) imprint on the Cosmic Microwave Background has many important advantages. The total SZ signal is an accurate and prec…

astro-ph.CO2013★ 185 cited

On the formation and physical properties of the Intra-Cluster Light in hierarchical galaxy formation models

E. Contini, G. De Lucia, A. Villalobos +1

We study the formation of the Intra-Cluster Light (ICL) using a semi-analytic model of galaxy formation, coupled to merger trees extracted from N-body simulations of groups and clu…

astro-ph.CO2013★ 28 cited

Constraining neutrino properties with a Euclid-like galaxy cluster survey

M. Costanzi Alunno Cerbolini, B. Sartoris, Jun-Qing Xia +3

We perform a forecast analysis on how well a Euclid-like photometric galaxy cluster survey will constrain the total neutrino mass and effective number of neutrino species. We base…

astro-ph.CO2012★ 905 cited

Cosmology and fundamental physics with the Euclid satellite

Luca Amendola, Stephen Appleby, David Bacon +60

Euclid is a European Space Agency medium class mission selected for launch in 2019 within the Cosmic Vision 2015-2025 programme. The main goal of Euclid is to understand the origin…

astro-ph.CO2011★ 35 cited

Statistics of Substructures in Dark Matter Haloes

E. Contini, G. De Lucia, S. Borgani

We study the amount and distribution of dark matter substructures within dark matter haloes, using a large set of high-resolution simulations ranging from group size to cluster siz…

astro-ph.CO2011★ 19 cited

Schmidt-Kennicutt relations in SPH simulations of disc galaxies with effective thermal feedback from supernovae

Pierluigi Monaco, Giuseppe Murante, Stefano Borgani +1

We study several versions of the Schmidt-Kennicutt (SK) relation obtained for isolated spiral galaxies in TreeSPH simulations run with the GADGET3 code including the novel MUlti-Ph…

astro-ph.CO2011★ 87 cited

Planck Early Results XXVI: Detection with Planck and confirmation by XMM-Newton of PLCK G266.6-27.3, an exceptionally X-ray luminous and massive galaxy cluster at z~1

Planck Collaboration, N. Aghanim, M. Arnaud +189

We present first results on PLCK G266.6-27.3, a galaxy cluster candidate detected at a signal-to-noise ratio of 5 in the Planck All Sky survey. An XMM-Newton validation observation…

astro-ph.CO2010★ 28 cited

Gas cooling in semi-analytic models and SPH simulations: are results consistent?

A. Saro, G. De Lucia, S. Borgani +1

We present a detailed comparison between the galaxy populations within a massive cluster, as predicted by hydrodynamical SPH simulations and by a semi-analytic model (SAM) of galax…

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-ph2001★ 97 cited

Pre-heating the ICM in high resolution simulations: the effect on the gas entropy

S. Borgani, F. Governato, J. Wadsley +5

We present results from high-resolution Tree+SPH simulations of galaxy clusters and groups, aimed at studying the effect of non-gravitational heating on the entropy of the ICM. We…

astro-ph2000

Optical/Infrared Survey of Galaxy Clusters

Luiz da Costa, S. Arnouts, S. Bardelli +13

In this contribution the ongoing effort to build a statistical sample of clusters of galaxies over a wide range of redshifts to study the evolution of clusters and member galaxies…

astro-ph1999★ 80 cited

Velocity Dispersions of CNOC Clusters and the Evolution of the Cluster Abundance

S. Borgani, M. Girardi, R. G. Carlberg +2

We present the results of the analysis of the internal velocity dispersions, σ_v, for the CNOC sample of distant galaxy clusters, based on an interlopers removal algorithm, which i…

astro-ph1993★ 10 cited

Large-Scale Clustering in Bubble Models

Luca Amendola, Stefano Borgani

We analyze the statistical properties of bubble models for the large-scale distribution of galaxies. To this aim, we realize static simulations, in which galaxies are mostly random…