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20172026
most citedThe LOFAR Two-metre Sky Survey -- V. Second data release

489 citations · 1.7k across the 66 of their papers we have counts for

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13 papers · 1 filter

astro-ph.HE2025

Crossing the veil of the brightest radio relic in the sky MACS J0717.6+3745

A. Pasetto, O. Vilchis, A. Bonafede +3

We present high-frequency, full-polarisation Jansky Very Large Array (VLA) radio data at X-band of the radio relic: MACS J0717.5+3745. Radio relics trace shock waves in the intracl…

astro-ph.HE2025★ 3 cited

The Advanced X-ray Imaging Satellite (AXIS) Community Science Book

Michael Koss, Nafisa Aftab, Steven W. Allen +395

The AXIS Community Science Book represents the collective effort of 592 scientists worldwide to define the transformative science enabled by the Advanced X-ray Imaging Satellite (A…

astro-ph.HE2025

PSZ2 G181.06+48.47 I: X-ray exploration of a low-mass cluster with exceptionally-distant radio relics

Andra Stroe, Kamlesh Rajpurohit, Zhenlin Zhu +13

Relics are diffuse, highly-polarized radio sources that trace merger-driven shocks at the periphery of merging galaxy clusters. The LOFAR survey recently discovered a rare example…

astro-ph.HE2024★ 9 cited

Probing particle acceleration in Abell 2256: from to 16 MHz to gamma rays

E. Osinga, R. J. van Weeren, G. Brunetti +9

Merging galaxy clusters often host spectacular diffuse radio synchrotron sources. These sources can be explained by a non-thermal pool of relativistic electrons accelerated by shoc…

astro-ph.HE2022★ 2 cited

The Coma cluster at LOFAR frequencies II: the halo, relic, and a new accretion relic

A. Bonafede, G. Brunetti, L. Rudnick +26

We present LOw Frequency ARray observations of the Coma cluster field at 144\,MHz. The cluster hosts one of the most famous radio halos, a relic, and a low surface-brightness bridg…

astro-ph.HE2021★ 33 cited

A MeerKAT-meets-LOFAR Study of MS 1455.0+2232: A 590 kiloparsec 'Mini'-Halo in a Sloshing Cool-Core Cluster

C. J. Riseley, K. Rajpurohit, F. Loi +13

Radio mini-haloes are poorly-understood, moderately-extended diffuse radio sources that trace the presence of magnetic fields and relativistic electrons on scales of hundreds of ki…

astro-ph.HE2021★ 27 cited

VLA Radio Study of a Sample of Nearby X-ray and Optically Bright Early-Type Galaxies

Romana Grossová, Norbert Werner, Francesco Massaro +9

Many massive early-type galaxies host central radio sources and hot X-ray atmospheres indicating the presence of radio-mechanical active galactic nucleus (AGN) feedback. The duty c…

astro-ph.HE2021★ 25 cited

Radio relics radio emission from multi-shock scenario

Giannandrea Inchingolo, Denis Wittor, Kamlesh Rajpurohit +1

Radio relics are giant (Mpc) synchrotron sources that are believed to be produced by the (re)acceleration of cosmic-ray electrons (CRe) by shocks in the intracluster medium.…

astro-ph.HE2021★ 23 cited

Morphology of radio relics II: Properties of polarised emission

P. Domínguez-Fernández, M. Brüggen, F. Vazza +7

Radio relics are diffuse radio sources in galaxy clusters that are associated with merger shock waves. Detailed observations of radio relics in total intensity and in polarisation…

astro-ph.HE2021★ 27 cited

A 3.5 Mpc-long radio relic in the galaxy cluster ClG 0217+70

D. N. Hoang, X. Zhang, C. Stuardi +14

Mega-parsec scale radio sources in the form of halos and relics are often detected in dynamically disturbed galaxy clusters. Although they are associated with merger-induced turbul…

astro-ph.HE2020★ 50 cited

Morphology of radio relics I: What causes the substructure of synchrotron emission?

P. Domínguez-Fernández, M. Brüggen, F. Vazza +5

High-resolution radio observations of cluster radio relics often show complex spatial and spectral features. However, it is not clear what these features reveal about the underlyin…

astro-ph.HE2020★ 39 cited

Discovering the most elusive radio relic in the sky: Diffuse Shock Acceleration caught in the act?

Nicola T. Locatelli, Kamlesh Rajpurohit, Franco Vazza +9

The origin of radio relics is usually explained via diffusive shock acceleration (DSA) or re-acceleration of electrons at/from merger shocks in galaxy clusters. The case of acceler…

astro-ph.HE2019★ 60 cited

New mysteries and challenges from the Toothbrush relic: wideband observations from 550 MHz to 8 GHz

K. Rajpurohit, M. Hoeft, F. Vazza +10

Radio relics are diffuse extended synchrotron sources that originate from shock fronts induced by galaxy cluster mergers. The actual particle acceleration mechanism at the shock fr…