activity
20092023
most citedSimulating the effect of AGN feedback on the metal enrichment of galaxy clusters

284 citations · 861 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2023★ 12 cited

Environmental dependence of AGN activity and star formation in galaxy clusters from Magneticum simulations

Gregor Rihtaršič, Veronica Biffi, Dunja Fabjan +1

(Abridged) Cluster environment has a strong impact on the star formation rate and AGN activity in cluster galaxies. In this work, we investigate the behaviour of different galaxy p…

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.CO2016★ 111 cited

Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution

N. Truong, E. Rasia, P. Mazzotta +11

We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable quantities such as X-ray luminosity,…

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★ 15 cited

Pointing to the minimum scatter: the generalized scaling relations for galaxy clusters

S. Ettori, E. Rasia, D. Fabjan +2

We introduce a generalized scaling law, M_tot = 10^K A^a B^b, to look for the minimum scatter in reconstructing the total mass of hydrodynamically simulated X-ray galaxy clusters,…

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…