activity
19982020
most citedNonthermal hard X-ray excess in the Coma cluster: resolving the discrepancy between the results of different PDS data analyses

38 citations · 51 across the 5 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2020

SuperModel Predictions in the Outskirts of the Galaxy Cluster Zwicky 3146

Roberto Fusco-Femiano

The relaxed galaxy cluster Zwicky 3146 is analyzed via the SuperModel, a tool already tested on many clusters since 2009. In particular, this analysis is focused on the intracluste…

astro-ph.CO2019★ 3 cited

Results from the SuperModel Analysis of the X-COP Galaxy Clusters Sample

Roberto Fusco-Femiano

In this work, the analysis of the stacked projected temperature profile of twelve galaxy clusters of the X-COP sample is performed via the SuperModel, a tool for investigating the…

astro-ph.CO2017

Nonthermal Pressure in the Outskirts of Abell 2142

R. Fusco-Femiano, A. Lapi

Clumping and turbulence are expected to affect the matter accreted onto the outskirts of galaxy clusters. To determine their impact on the thermodynamic properties of Abell 2142 we…

astro-ph.CO2016

The Intragroup versus the Intracluster Medium

A. Cavaliere, R. Fusco-Femiano, A. Lapi

Galaxy groups differ from clusters primarily by way of their lower masses, M~10^14 M_sun vs. M~10^15 M_sun. We discuss how mass affects the thermal state of the intracluster or the…

astro-ph2008★ 1 cited

Comments to the review "Nonthermal phenomena in clusters of galaxies" by Y.Rephaeli et al. that will appear on the book: Clusters of galaxies: beyond the thermal view

Roberto Fusco-Femiano, Mauro Orlandini

Comments to the review "Nonthermal Phenomena in Clusters of Galaxies" by Y.Rephaeli et al. (arXiv:0801.0982 [astro-ph]) that regard the presence of a hard X-ray excess in the Coma…

astro-ph2007★ 9 cited

XMM-Newton observation of the cluster ZW 1305.4+2941 in the field SA 57

Fabio Gastaldello, Dario Trevese, Fausto Vagnetti +1

We report the details of an XMM observation of the cluster of galaxies ZW 1305.4+2941 at the intermediate redshift of z=0.241, increasing the small number of interesting X-ray cons…