activity
20042026
most citedLOFAR: The LOw-Frequency ARray

2.7k citations · 8.2k across the 161 of their papers we have counts for

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Showing 2016Show all

10 papers · 1 filter

astro-ph.GA2016★ 90 cited

Faraday tomography of the local interstellar medium with LOFAR: Galactic foregrounds towards IC342

C. L. Van Eck, M. Haverkorn, M. I. R. Alves +18

The new generation of low-frequency radio telescopes, such as the Low Frequency Array (LOFAR: a Square Kilometre Array-low pathfinder), provides advancements in our capability of p…

astro-ph.SR2016★ 13 cited

A LOFAR detection of the low mass young star T Tau at 149 MHz

Colm P. Coughlan, Rachael E. Ainsworth, Jochen Eislöffel +15

Radio observations of young stellar objects (YSOs) enable the study of ionised plasma outflows from young protostars via their free-free radiation. Previous studies of the low-mass…

astro-ph.CO2016★ 16 cited

Diffuse radio emission in MACS J0025.41222: the effect of a major merger on bulk separation of ICM components

C. J. Riseley, A. M. M. Scaife, M. W. Wise +1

Mergers of galaxy clusters are among the most energetic events in the Universe. These events have significant impact on the intra-cluster medium, depositing vast amounts of energy…

astro-ph.HE2016★ 49 cited

Flares, wind and nebulae: the 2015 December mini-outburst of V404 Cygni

T. Muñoz-Darias, J. Casares, D. Mata Sánchez +22

After more than 26 years in quiescence, the black hole transient V404 Cyg went into a luminous outburst in June 2015, and additional activity was detected in late December of the s…

astro-ph.GA2016★ 16 cited

The Discovery of a Low-Luminosity SPIRAL DRAGN

D. D. Mulcahy, M. Y. Mao, I. Mitsuishi +7

Standard galaxy formation models predict that large-scale double-lobed radio sources, known as DRAGNs, will always be hosted by elliptical galaxies. In spite of this, in recent yea…

astro-ph.GA2016★ 6 cited

A GMRT survey of regions towards the Taurus Molecular Cloud at 323 and 608 MHz

Rachael E. Ainsworth, Colm P. Coughlan, David A. Green +2

We present observations of three active sites of star formation in the Taurus Molecular Cloud complex taken at 323 and 608 MHz (90 and 50 cm, respectively) with the Giant Metrewave…