activity
20102015
most citedMORESANE: MOdel REconstruction by Synthesis-ANalysis Estimators. A sparse deconvolution algorithm for radio interferometric imaging

66 citations · 110 across the 8 of their papers we have counts for

collaborators
Showing astro-ph.COShow all

5 papers · 1 filter

astro-ph.CO20152 cited

Statistical methods for the analysis of rotation measure grids in large scale structures in the SKA era

Valentina Vacca, Niels Oppermann, Torsten Ensslin +18

To better understand the origin and properties of cosmological magnetic fields, a detailed knowledge of magnetic fields in the large-scale structure of the Universe (galaxy cluster…

astro-ph.CO20156 cited

Cluster magnetic fields through the study of polarized radio halos in the SKA era

F. Govoni, M. Murgia, H. Xu +17

Galaxy clusters are unique laboratories to investigate turbulent fluid motions and large scale magnetic fields. Synchrotron radio halos at the center of merging galaxy clusters pro…

astro-ph.CO20141 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.CO2014

The SKA view of cool-core clusters: evolution of radio mini-halos and AGN feedback

Myriam Gitti, Paolo Tozzi, Gianfranco Brunetti +10

In about 70% of the population of relaxed, cool-core galaxy clusters, the brightest cluster galaxy (BCG) is radio loud, showing non-thermal radio jets and lobes ejected by the cent…

astro-ph.CO2010

Non-thermal emission from galaxy clusters: a Pandora's vase for astrophysics

C. Ferrari

The existence of cosmic rays and weak magnetic fields in the intracluster volume has been well proven by deep radio observations of galaxy clusters. However a detailed physical cha…