activity
20042009
most citedA low-frequency radio halo associated with a cluster of galaxies

255 citations · 2k across the 19 of their papers we have counts for

collaborators

16 papers

astro-ph.CO20092 cited

The GMRT Radio Halo Survey and low frequency follow-up

T. Venturi, S. Giacintucci, R. Cassano +6

The GMRT Radio Halo Survey, carried out at 610 MHz to investigate the statistical properties of cluster radio halos in a complete cluster sample selected in the redshift interval z…

astro-ph.CO20093 cited

Large-scale diffuse radio emission from clusters of galaxies and the importance of low frequency radio observations

Rossella Cassano

The presence of non-thermal components in galaxy clusters is now clearly established. Diffuse radio emission from the Intra Cluster Medium (ICM) of several galaxy clusters is revea…

astro-ph.HE20094 cited

High energy emission from galaxy clusters and particle acceleration due to MHD turbulence

G. Brunetti, P. Blasi, R. Cassano +1

In the next years the FERMI gamma ray telescope and the Cherenkov telescopes will put very stringent constraints to models of gamma ray emission from galaxy clusters providing cruc…

astro-ph20083 cited

Gamma ray emission and stochastic particle acceleration in galaxy clusters

G. Brunetti, P. Blasi, R. Cassano +1

FERMI (formely GLAST) will shortly provide crucial information on relativistic particles in galaxy clusters. We discuss non-thermal emission in the context of general calculations…

astro-ph2008255 cited

A low-frequency radio halo associated with a cluster of galaxies

G. Brunetti, S. Giacintucci, R. Cassano +7

Clusters of galaxies are the largest gravitationally bound objects in the Universe, containing about 10^15 solar masses of hot (10^8 K) gas, galaxies and dark matter in a typical v…

astro-ph200847 cited

A morphological comparison between giant radio halos and radio mini--halos in galaxy clusters

R. Cassano, M. Gitti, G. Brunetti

In this letter we present a morphological comparison between giant radio halos and radio mini-halos in galaxy clusters based on radio--X-ray luminosity, P_{1.4}-L_X, and radio lumi…