activity
19982020
most citedHard X-Ray Radiation in the Coma Cluster Spectrum

260 citations · 954 across the 30 of their papers we have counts for

collaborators

30 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★ 9 cited

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★ 2 cited

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-ph.CO2014★ 4 cited

SuperModel Analysis of Abell 1246 and J255: on the Evolution of Galaxy Clusters from High to Low Entropy States

R. Fusco-Femiano, A. Lapi

We present an analysis of high-quality X-ray data out to the virial radius for the two galaxy clusters Abell 1246 and GMBCG J255.34805+64.23661 (J255) by means of our entropy-based…

astro-ph.CO2014★ 18 cited

Entropy Flattening, Gas Clumping and Turbulence in Galaxy Clusters

R. Fusco-Femiano, A. Lapi

Several physical processes and formation events are expected in cluster outskirts, a vast region up to now essentially not covered by observations. The recent Suzaku (X-ray) and Pl…

astro-ph.CO2013★ 14 cited

Turbulence in the SuperModel: Mass Reconstruction with Nonthermal Pressure for Abell 1835

R. Fusco-Femiano, A. Lapi

The total mass derived from X-ray emission is biased low in a large number of clusters when compared with the mass estimated via strong and weak lensing. Suzaku and Chandra observa…

astro-ph.CO2012★ 11 cited

The Planck Sunyaev-Zel'dovich vs. the X-ray View of the Coma Cluster

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

The Planck collaboration has recently published precise and resolved measurements of the Sunyaev-Zel'dovich effect in Abell 1656 (the Coma cluster of galaxies), so directly gauging…

astro-ph.CO2011★ 20 cited

A Grand Design for Galaxy Clusters: Connections and Predictions

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

We take up from a library of 12 galaxy clusters featuring extended X-ray observations of their Intra Cluster Plasma (ICP), analyzed with our entropy-based Supermodel. Its few intri…

astro-ph.CO2011★ 11 cited

Supermodel Analysis of the Hard X-Ray Excess in the Coma Cluster

Roberto Fusco-Femiano, Mauro Orlandini, Massimiliano Bonamente +1

The Supermodel provides an accurate description of the thermal contribution by the hot intracluster plasma which is crucial for the analysis of the hard excess. In this paper the t…

astro-ph.CO2010★ 26 cited

Non Thermal Support for the Outer Intracluster Medium

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

We submit that non thermalized support for the outer intracluster medium in relaxed galaxy clusters is provided by turbulence, driven by inflows of intergalactic gas across the vir…

astro-ph.CO2010★ 44 cited

Probing the Astrophysics of Cluster Outskirts

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

In galaxy clusters the entropy distribution of the IntraCluster Plasma modulates the latter's equilibrium within the Dark Matter gravitational wells, as rendered by our Supermodel.…

astro-ph.CO2009★ 32 cited

Galaxy Clusters, a Novel Look at Diffuse Baryons Withstanding Dark Matter Gravity

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

[abridged] The equilibria of the intracluster plasma (ICP) and of the gravitationally dominant dark matter (DM) are governed by the hydrostatic and the Jeans equation. Jeans, with…

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…

astro-ph2007

Hard X-Ray Excess in the Coma Cluster: a Reply to Rossetti & Molendi (astro-ph/0702417)

Roberto Fusco-Femiano, Raffaella Landi, Mauro Orlandini

A short replay to the comment of Rossetti & Molendi (astro-ph/0702417) in answer to the paper of Fusco-Femiano, Landi & Orlandini 2007 regarding the presence of a nonthermal compon…

astro-ph2006★ 38 cited

Nonthermal hard X-ray excess in the Coma cluster: resolving the discrepancy between the results of different PDS data analyses

Roberto Fusco-Femiano, Raffaella Landi, Mauro Orlandini

The detection of a nonthermal excess in the Coma cluster spectrum by two BeppoSAX observations analyzed with the XAS package (Fusco-Femiano et al.) has been disavowed by an analysi…

astro-ph2005★ 31 cited

Nonthermal hard X-ray excess in the cluster Abell 2256 from two epoch observations

Roberto Fusco-Femiano, Raffaella Landi, Mauro Orlandini

After confirmation of the presence of a nonthermal hard X-ray excess with respect to the thermal emission in the Coma cluster from two independent observations, obtained using the…

astro-ph2003★ 125 cited

Confirmation of non-thermal hard X-ray excess in the Coma cluster from two epoch observations

Roberto Fusco-Femiano, Mauro Orlandini, Gianfranco Brunetti +4

We report the hard X-ray spectrum of the Coma cluster obtained using the PDS data of two independent BeppoSAX observations performed with a time interval of about three years. In b…

astro-ph2002★ 34 cited

Hard X-ray and radio observations of Abell 754

R. Fusco-Femiano, M. Orlandini, S. De Grandi +5

We present a long BeppoSAX observation of Abell 754 that reports a nonthermal excess with respect to the thermal emission at energies greater than ~45 keV. A VLA radio observation…

astro-ph2002★ 25 cited

Detection of X-ray Emission from the Eastern Radio Lobe of PICTOR A

Paola Grandi, Matteo Guainazzi, Laura Maraschi +5

The XMM-Newton satellite has revealed extended X-ray emission from the eastern radio lobe of the Fanaroff-Riley II Radio Galaxy Pictor A. The X-ray spectrum, accumulated on a regio…

astro-ph2002

Development of Hydrodynamic Instability in the Intergalactic Medium of the Merging Cluster of Galaxies A3667

Pasquale Mazzotta, Alexey Vikhlinin, Roberto Fusco-Femiano +1

A3667, a spectacular merger cluster, was observed by Chandra twice. In this paper we review the main results of the analysis of these observations. In particular we show evidence f…

astro-ph2001★ 45 cited

Hard X-ray emission from the galaxy cluster A3667

R. Fusco-Femiano, D. Dal Fiume, M. Orlandini +3

We report the results of a long BeppoSAX observation of Abell 3667, one of the most spectacular galaxy cluster in the southern sky. A clear detection of hard X-ray radiation up to…

astro-ph2000★ 118 cited

Hard X-ray emission from the galaxy cluster A2256

R. Fusco-Femiano, D. Dal Fiume, S. De Grandi +6

After the positive detection by BeppoSAX of hard X-ray radiation up to ~80 keV in the Coma cluster spectrum, we present evidence for nonthermal emission from A2256 in excess of the…