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20112026
most citedThe LOFAR Two-metre Sky Survey - II. First data release

586 citations · 5.2k across the 112 of their papers we have counts for

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Showing 2021Show all

16 papers · 1 filter

astro-ph.GA2021★ 16 cited

The GLEAMing of the First Supermassive Black Holes

Guillaume Drouart, Nick Seymour, Tim J. Galvin +7

We present the results of a new selection technique to identify powerful (WHz) radio galaxies towards the end of the Epoch of Reionisation. Our m…

astro-ph.SR2021★ 23 cited

The TESS View of LOFAR Radio-Emitting Stars

Benjamin J. S. Pope, Joseph R. Callingham, Adina D. Feinstein +4

The recent detection of the M dwarf GJ 1151 at 144 MHz low radio frequencies using LOFAR has been interpreted as evidence of an exoplanet magnetically interacting with its host sta…

astro-ph.SR2021★ 9 cited

Radio modelling of the brightest and most luminous non-thermal colliding-wind binary Apep

S. Bloot, J. R. Callingham, B. Marcote

Apep is the brightest and most luminous non-thermal colliding-wind binary by over an order of magnitude. It has been suggested from infrared observations that one of the Wolf-Rayet…

astro-ph.SR2021★ 90 cited

The population of M dwarfs observed at low radio frequencies

J. R. Callingham, H. K. Vedantham, T. W. Shimwell +12

Coherent low-frequency ( MHz) radio emission from stars encodes the conditions of the outer corona, mass-ejection events, and space weather. Previous low-frequency se…

astro-ph.GA2021★ 16 cited

High-resolution international LOFAR observations of 4C~43.15 -- Spectral ages and injection indices in a high-z radio galaxy

Frits Sweijen, Leah K. Morabito, Jeremy Harwood +6

Radio sources with steep spectra are preferentially associated with the most distant galaxies, the relation, but the reason for this relation is an open question. The spatial…

astro-ph.GA2021★ 25 cited

Origin of the ring structures in Hercules A -- Sub-arcsecond 144 MHz to 7 GHz observations

R. Timmerman, R. J. van Weeren, J. R. Callingham +18

The prominent radio source Hercules A features complex structures in its radio lobes. Although it is one of the most comprehensively studied sources in the radio sky, the origin of…

astro-ph.GA2021★ 35 cited

Sub-arcsecond imaging with the International LOFAR Telescope: II. Completion of the LOFAR Long-Baseline Calibrator Survey

Neal Jackson, Shruti Badole, John Morgan +69

The Low-Frequency Array (LOFAR) Long-Baseline Calibrator Survey (LBCS) was conducted between 2014 and 2019 in order to obtain a set of suitable calibrators for the LOFAR array. In…

astro-ph.IM2021★ 88 cited

Sub-arcsecond imaging with the International LOFAR Telescope I. Foundational calibration strategy and pipeline

L. K. Morabito, N. J. Jackson, S. Mooney +71

[abridged] The International LOFAR Telescope is an interferometer with stations spread across Europe. With baselines of up to ~2,000 km, LOFAR has the unique capability of achievin…

astro-ph.GA2021★ 15 cited

Pushing subarcsecond resolution imaging down to 30 MHz with the trans-European International LOFAR Telescope

C. Groeneveld, R. J. van Weeren, G. K. Miley +12

Relatively little information is available about the Universe at ultra-low radio frequencies, i.e. below 50 MHz (ULF), although the ULF spectral window contains a wealth of unique…

astro-ph.GA2021★ 7 cited

The GLEAM 200 MHz Local Radio Luminosity Function for AGN and Star-forming Galaxies

T. M. O. Franzen, N. Seymour, E. M. Sadler +24

The GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) is a radio continuum survey at 76-227 MHz of the entire southern sky (Declination ) with an angular…

astro-ph.SR2021★ 28 cited

Coherent radio emission from a population of RS Canum Venaticorum systems

S. E. B. Toet, H. K. Vedantham, J. R. Callingham +5

Coherent radio emission from stars can be used to constrain fundamental coronal plasma parameters, such as plasma density and magnetic field strength. It is also a probe of chromos…

astro-ph.SR2021

Evidence for cold plasma in planetary nebulae from radio observations with the LOw Frequency ARray (LOFAR)

Marcin Hajduk, Marijke Haverkorn, Timothy Shimwell +6

We present observations of planetary nebulae with the LOw Frequency ARray (LOFAR) between 120 and 168 MHz. The images show thermal free-free emission from the nebular shells. We ha…

astro-ph.SR2021★ 6 cited

Detection of coherent low-frequency radio bursts from weak-line TTauri stars

A. Feeney-Johansson, S. J. D. Purser, T. P. Ray +7

In recent years, thanks to new facilities such as LOFAR capable of sensitive observations, much work has been done on the detection of stellar radio emission at low frequencies. Su…

astro-ph.SR2021★ 15 cited

Large closed-field corona of WX UMa evidenced from radio observations

I. Davis, H. K. Vedantham, J. R. Callingham +5

The space-weather conditions that result from stellar winds significantly impact the habitability of exoplanets. The conditions can be calculated from first principles if the neces…

astro-ph.IM2021★ 100 cited

The LOFAR LBA Sky Survey I. survey description and preliminary data release

F. de Gasperin, W. L. Williams, P. Best +38

LOFAR is the only radio telescope that is presently capable of high-sensitivity, high-resolution (<1 mJy/b and <15") observations at ultra-low frequencies (<100 MHz). To utilise th…

astro-ph.SR2021★ 49 cited

Low-frequency monitoring of flare star binary CR Draconis: Long-term electron-cyclotron maser emission

J. R. Callingham, B. J. S. Pope, A. D. Feinstein +12

Recently detected coherent low-frequency radio emission from M dwarf systems shares phenomenological similarities with emission produced by magnetospheric processes from the gas gi…