activity
20092025
most citedThe LOFAR Two-metre Sky Survey - I. Survey Description and Preliminary Data Release

654 citations · 4.6k across the 70 of their papers we have counts for

collaborators
Showing 2018Show all

8 papers · 1 filter

astro-ph.GA2018★ 17 cited

The first detection of radio recombination lines at cosmological distances

K. L. Emig, P. Salas, F. de Gasperin +4

Recombination lines involving high principal quantum numbers populate the radio spectrum in large numbers. Low-frequency (<1 GHz) observations of radio recombination lines (RRLs) p…

astro-ph.GA2018★ 586 cited

The LOFAR Two-metre Sky Survey - II. First data release

T. W. Shimwell, C. Tasse, M. J. Hardcastle +104

The LOFAR Two-metre Sky Survey (LoTSS) is an ongoing sensitive, high-resolution 120-168MHz survey of the entire northern sky for which observations are now 20% complete. We present…

astro-ph.HE2018★ 17 cited

A low-frequency view of mixed-morphology supernova remnant VRO 42.05.01, and its neighbourhood

M. Arias, J. Vink, M. Iacobelli +7

Mixed-morphology supernova remnants (MM SNRs) are a mysterious class of objects that display thermal X-ray emission within their radio shell. They are an older class of SNRs, and a…

astro-ph.GA2018★ 24 cited

Cooling in the X-ray halo of the rotating, massive early-type galaxy NGC 7049

A. Juráňová, N. Werner, M. Gaspari +9

The relative importance of the physical processes shaping the thermodynamics of the hot gas permeating rotating, massive early-type galaxies is expected to be different from that i…

astro-ph.GA2018★ 124 cited

A Galaxy-Scale Fountain of Cold Molecular Gas Pumped by a Black Hole

Grant R. Tremblay, Françoise Combes, J. B. Raymond Oonk +36

We present ALMA and MUSE observations of the Brightest Cluster Galaxy in Abell 2597, a nearby (z=0.0821) cool core cluster of galaxies. The data map the kinematics of a three billi…

astro-ph.HE2018★ 46 cited

Low-Frequency Radio Absorption in Cassiopeia A

M. Arias, J. Vink, F. de Gasperin +3

Cassiopeia A is one of the best-studied supernova remnants. Its shocked ejecta emits brightly in radio and X-rays. Its unshocked ejecta can be studied through infrared emission, th…