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

489 citations · 1k across the 23 of their papers we have counts for

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Showing astro-ph.HEShow all

11 papers · 1 filter

astro-ph.HE2025★ 1 cited

Discovery of large-scale radio emission enveloping the mini-halo in the most X-ray luminous galaxy cluster RX~J1347.5-1145

D. N. Hoang, M. Brüggen, A. Bonafede +8

Diffuse radio sources, known as mini-halos and halos, are detected at the centres of galaxy clusters. These centralized diffuse sources are typically observed individually, with bo…

astro-ph.HE2024★ 18 cited

The LOFAR-eFEDS survey: The incidence of radio and X-ray AGN and the disk-jet connection

Z. Igo, A. Merloni, D. Hoang +15

Radio jets are present in a diverse sample of AGN. However, the mechanisms of jet powering are not fully understood, and it is yet unclear to what extent they obey mass-invariant s…

astro-ph.HE2023★ 12 cited

A search for inter-cluster filaments with LOFAR and eROSITA

D. N. Hoang, M. Brüggen, T. W. Shimwell +13

Cosmological simulations predict the presence of warm hot thermal gas in the cosmic filaments that connect galaxy clusters. This gas is thought to constitute an important part of t…

astro-ph.HE2021

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.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.HE2020★ 46 cited

Radio observations of the merging galaxy cluster system Abell 3391-Abell 3395

M. Brüggen, T. H. Reiprich, E. Bulbul +20

The pre-merging system of galaxy clusters Abell 3391-Abell 3395 located at a mean redshift of 0.053 has been observed at 1 GHz in an ASKAP/EMU Early Science observation as well as…