activity
20182022
most citedThe LOFAR Two-metre Sky Survey -- V. Second data release

489 citations · 1.2k across the 14 of their papers we have counts for

collaborators

18 papers

astro-ph.GA202252 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.GA2022489 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.GA202266 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…

astro-ph.GA2021

The Nature of Hyperluminous Infrared Galaxies

F. Gao, L. Wang, A. Efstathiou +7

We make use of multi-wavelength data of a large hyperluminous infrared (HLIRG) sample to derive their main physical properties, e.g., stellar mass, star-formation rate (SFR), volum…

astro-ph.GA20217 cited

Low-frequency radio spectra of submillimetre galaxies in the Lockman Hole

J. Ramasawmy, J. E. Geach, M. J. Hardcastle +19

We investigate the radio properties of a sample of 53 sources selected at 850 m from the SCUBA-2 Cosmology Legacy Survey using new deep, low-frequency radio imaging of the Lockm…

astro-ph.IM2020248 cited

The LOFAR Two Meter Sky Survey: Deep Fields, I -- Direction-dependent calibration and imaging

C. Tasse, T. Shimwell, M. J. Hardcastle +29

The Low Frequency Array (LOFAR) is an ideal instrument to conduct deep extragalactic surveys. It has a large field of view and is sensitive to large scale and compact emission. It…