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20182026
most citedThe LOFAR Two-metre Sky Survey -- V. Second data release

489 citations · 1k across the 15 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2025

The Peculiar Mini-Halo in the Shapley Supercluster Member Abell 3558

K. S. Trehaeven, T. Venturi, O. Smirnov +9

We present a multi-band study of the diffuse emission in the galaxy cluster Abell 3558, located in the core of the Shapley Supercluster. Using new MeerKAT UHF-Band and uGMRT Band-3…

astro-ph.GA2022★ 489 cited

The LOFAR Two-metre Sky Survey -- V. Second data release

T. W. Shimwell, M. J. Hardcastle, C. Tasse +103

In this data release from the LOFAR Two-metre Sky Survey (LoTSS) we present 120-168MHz images covering 27% of the northern sky. Our coverage is split into two regions centred at ap…

astro-ph.GA2020★ 22 cited

The great Kite in the sky: a LOFAR observation of the radio source in Abell 2626

A. Ignesti, T. Shimwell, G. Brunetti +15

The radio source at the center of the galaxy cluster Abell 2626, also known as the Kite, stands out for its unique morphology composed of four, symmetric arcs. Previous studies hav…

astro-ph.GA2020★ 86 cited

The beautiful mess in Abell 2255

A. Botteon, G. Brunetti, R. J. van Weeren +18

We present LOFAR observations of one of the most spectacular objects in the radio sky: Abell 2255. This is a nearby () merging galaxy cluster hosting one of the first r…

astro-ph.GA2019★ 20 cited

LOFAR discovery of a radio halo in the high-redshift galaxy cluster PSZ2 G099.86+58.45

R. Cassano, A. Botteon, G. Di Gennaro +15

In this Letter, we report the discovery of a radio halo in the high-redshift galaxy cluster PSZ2 G099.86+58.45 () with the LOw Frequency ARray (LOFAR) at 120-168 MHz. This…

astro-ph.GA2018★ 85 cited

Deep Very Large Array observations of the merging cluster CIZA J2242.8+5301: continuum and spectral imaging

G. Di Gennaro, R. J. van Weeren, M. Hoeft +14

Despite progress in understanding radio relics, there are still open questions regarding the underlying particle acceleration mechanisms. In this paper we present deep 1--4 GHz VLA…