activity
19952026
most citedTurbulent Motions and Shocks Waves in Galaxy Clusters simulated with AMR

212 citations · 2.4k across the 62 of their papers we have counts for

collaborators

62 papers

astro-ph.GA2026

Simulating megaparsec-scale jets of radio galaxies: Magneto-hydrodynamics of jets reaching 5 Mpc

Gourab Giri, Dario Borgogno, Marco Tavani +9

Extragalactic jets have long prompted the question of how far relativistic outflows can extend, with some radio sources reaching 5 - 7 Mpc in length. These great extents motivate i…

astro-ph.HE2025★ 13 cited

The evolution of cosmic ray electrons in the cosmic web: seeding by AGN, star formation and shocks

F. Vazza, C. Gheller, F Zanetti +4

Several processes in the Universe convert a fraction of gas kinetic energy into the acceleration of relativistic electrons, making them observable at radio wavelengths, or contribu…

astro-ph.HE2023

Efficiency of turbulent reacceleration by solenoidal turbulence and its application to the origin of radio mega halos in cluster outskirts

Kosuke Nishiwaki, Gianfranco Brunetti, Franco Vazza +1

Recent radio observations with Low-Frequency Array (LOFAR) discovered diffuse emission extending beyond the scale of classical radio halos. The presence of such mega halos indicate…

astro-ph.IM2023★ 22 cited

SKA Science Data Challenge 2: analysis and results

P. Hartley, A. Bonaldi, R. Braun +105

The Square Kilometre Array Observatory (SKAO) will explore the radio sky to new depths in order to conduct transformational science. SKAO data products made available to astronomer…

astro-ph.IM2023

High Performance W-stacking for Imaging Radio Astronomy Data: a Parallel and Accelerated Solution

Claudio Gheller, Giuliano Taffoni, David Goz

Current and upcoming radio-interferometers are expected to produce volumes of data of increasing size that need to be processed in order to generate the corresponding sky brightnes…

astro-ph.CO2022★ 52 cited

Magnetic field evolution in cosmic filaments with LOFAR data

E. Carretti, S. O'Sullivan, V. Vacca +4

Measuring the magnetic field in cosmic filaments reveals how the Universe is magnetised and the process that magnetised it. Using the Rotation Measures (RM) at 144-MHz from the LoT…