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

489 citations · 1.8k across the 43 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.IM2022★ 211 cited

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Shoko Jin, Scott C. Trager, Gavin B. Dalton +212

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree…

astro-ph.GA2022★ 39 cited

Identifying active galactic nuclei via brightness temperature with sub-arcsecond International LOFAR Telescope observations

Leah K. Morabito, F. Sweijen, J. F. Radcliffe +11

Identifying active galactic nuclei (AGN) and isolating their contribution to a galaxy's energy budget is crucial for studying the co-evolution of AGN and their host galaxies. Brigh…

astro-ph.IM2022★ 18 cited

A machine learning classifier for LOFAR radio galaxy cross-matching techniques

Lara Alegre, Jose Sabater, Philip Best +7

New-generation radio telescopes like LOFAR are conducting extensive sky surveys, detecting millions of sources. To maximise the scientific value of these surveys, radio source comp…

astro-ph.GA2022★ 52 cited

Cosmic evolution of low-excitation radio galaxies in the LOFAR Two-meter Sky Survey Deep Fields

R. Kondapally, P. N. Best, R. K. Cochrane +16

Feedback from low-excitation radio galaxies (LERGs) plays a key role in the lifecycle of massive galaxies in the local Universe; their evolution, and the impact of these active gal…

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.GA2022★ 66 cited

Accretion mode versus radio morphology in the LOFAR Deep Fields

B. Mingo, J. H. Croston, P. N. Best +17

Radio-loud active galaxies have two accretion modes [radiatively inefficient (RI) and radiatively efficient (RE)], with distinct optical and infrared signatures, and two jet dynami…