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19932026
most citedA New Radio - X-Ray Probe of Galaxy Cluster Magnetic Fields

541 citations · 5k across the 101 of their papers we have counts for

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31 papers · 1 filter

astro-ph.CO2026

Extended radio emission in and around the merging cluster A520 as seen by MeerKAT

S. Giacintucci, W. D. Cotton, M. Markevitch +3

We present results from a deep MeerKAT 1.28 GHz observation of Abell 520, a galaxy cluster in the middle of a merger and a treasure trove of merger-generated phenomena. MeerKAT's c…

astro-ph.CO2022★ 33 cited

The detection of cluster magnetic fields via radio source depolarisation

E. Osinga, R. J. van Weeren, F. Andrade-Santos +7

It has been well established that galaxy clusters have magnetic fields. The exact properties and origin of these magnetic fields are still uncertain even though these fields play a…

astro-ph.CO2021★ 69 cited

MeerKAT view of the diffuse radio sources in Abell 3667 and their interactions with the thermal plasma

F. de Gasperin, L. Rudnick, A. Finoguenov +11

During their lifetime, galaxy clusters grow through the accretion of matter from the filaments of the large scale structure and from mergers with other clusters. These mergers rele…

astro-ph.CO2021★ 25 cited

Turbulent magnetic fields in the merging galaxy cluster MACS J0717.5+3745: polarization analysis

K. Rajpurohit, M. Hoeft, D. Wittor +20

We present wideband polarimetric observations, obtained with the Karl G. Jansky Very Large Array (VLA), of the merging galaxy cluster MACS J0717.5+3745, which hosts one of the most…

astro-ph.CO2019★ 27 cited

An ALMA+ACA measurement of the shock in the Bullet Cluster

Luca Di Mascolo, Tony Mroczkowski, Eugene Churazov +9

The thermal Sunyaev-Zeldovich (SZ) effect presents a relatively new tool for characterizing galaxy cluster merger shocks, traditionally studied through X-ray observations. Widely r…

astro-ph.CO2018★ 51 cited

Observations of a nearby filament of galaxy clusters with the Sardinia Radio Telescope

V. Vacca, M. Murgia, F. Govoni +29

We report the detection of diffuse radio emission which might be connected to a large-scale filament of the cosmic web covering a 8deg x 8deg area in the sky, likely associated wit…