activity
20182022
most citedMagnetic field strength in cosmic web filaments

62 citations · 268 across the 8 of their papers we have counts for

collaborators

13 papers

astro-ph.CO202262 cited

Magnetic field strength in cosmic web filaments

E. Carretti, V. Vacca, S. P. O'Sullivan +8

We used the Rotation Measure (RM) catalogue derived from the LOFAR Two-metre Sky Survey Data Release 2 (LoTSS DR2) at 144-MHz to measure the evolution with redshift of the extragal…

astro-ph.GA202147 cited

The intra-cluster magnetic field in the double relic galaxy cluster Abell 2345

C. Stuardi, A. Bonafede, L. Lovisari +5

Magnetic fields are ubiquitous in galaxy clusters, yet their radial profile, power spectrum, and connection to host cluster properties are poorly known. Merging galaxy clusters hos…

astro-ph.GA20206 cited

Peering Into the Extended X-ray Emission on Megaparsec Scale in 3C 187

A. Paggi, F. Massaro, H. A. Pena-Herazo +7

Context. The diffuse X-ray emission surrounding radio galaxies is generally interpreted either as due to inverse Compton scattering of non-thermal radio-emitting electrons on the C…

astro-ph.CO202057 cited

The Coma cluster at LOFAR frequencies I: insights into particle acceleration mechanisms in the radio bridge

A. Bonafede, G. Brunetti, F. Vazza +18

Radio synchrotron emission from the bridges of low-density gas connecting galaxy clusters and groups is a challenge for particle acceleration processes. In this work, we analyse th…

astro-ph.HE202012 cited

Extended X-ray emission around FR II radio galaxies: hotspots, lobes and galaxy clusters

Ana Jimenez-Gallardo, Francesco Massaro, Alessandro Paggi +20

We present a systematic analysis of the extended X-ray emission discovered around 35 FR II radio galaxies from the revised Third Cambridge catalog (3CR) Chandra Snapshot Survey wit…

astro-ph.HE20209 cited

ClG 0217+70: A massive merging galaxy cluster with a large radio halo and relics

X. Zhang, A. Simionescu, J. S. Kaastra +7

We present an analysis of archival Chandra data of the merging galaxy cluster ClG 0217+70. The Fe XXV He X-ray emission line is clearly visible in the 25 ks observation, allowin…