activity
20162026
most citedThe LOFAR Two-metre Sky Survey -- V. Second data release

489 citations · 1.6k across the 34 of their papers we have counts for

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Showing 2021Show all

7 papers · 1 filter

astro-ph.CO2021★ 133 cited

The eROSITA Final Equatorial-Depth Survey (eFEDS): Catalog of galaxy clusters and groups

A. Liu, E. Bulbul, V. Ghirardini +31

The eROSITA Final Equatorial-Depth Survey has been carried out during the PV phase of the SRG/eROSITA telescope and completed in November 2019. This survey is designed to provide t…

astro-ph.CO2021★ 41 cited

Studying the merging cluster Abell 3266 with eROSITA

J. S. Sanders, V. Biffi, M. Brüggen +15

Abell 3266 is one of the X-ray brightest galaxy clusters in the sky and is a well-known merging system. Using the ability of the eROSITA telescope onboard SRG (Spectrum Röntgen Gam…

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.CO2021★ 19 cited

Discovery of a radio halo (and relic) in a M cluster

A. Botteon, R. Cassano, R. J. van Weeren +12

Radio halos are diffuse synchrotron sources observed in dynamically unrelaxed galaxy clusters. Current observations and models suggest that halos trace turbulent regions in the int…

astro-ph.HE2021★ 21 cited

Radio relics in PSZ2 G096.88+24.18: A connection with pre-existing plasma

A. Jones, F. de Gasperin, V. Cuciti +10

Giant radio relics are arc-like structures of diffuse, non-thermal synchrotron radiation that trace shock waves induced by galaxy cluster mergers. The particle (re-)acceleration me…

astro-ph.GA2021★ 31 cited

Downstream depolarization in the Sausage relic: a 1-4 GHz Very Large Array study

G. Di Gennaro, R. J. van Weeren, L. Rudnick +10

Radio relics are elongated sources related to shocks driven by galaxy cluster merger events. Although these objects are highly polarized at GHz frequencies (), high-r…