activity
20172019
most citedLOFAR observations of decameter carbon radio recombination lines towards Cassiopeia A

25 citations · 55 across the 3 of their papers we have counts for

collaborators

6 papers

astro-ph.IM20197 cited

Searching for the largest bound atoms in space

K. L. Emig, P. Salas, F. de Gasperin +5

(abridged) Radio recombination lines (RRLs) at frequencies < 250 MHz trace the cold, diffuse phase of the ISM. Next generation low frequency interferometers, such as LOFAR, MWA…

astro-ph.GA201923 cited

Carbon radio recombination lines from gigahertz to megahertz frequencies towards Orion A

P. Salas, J. B. R. Oonk, K. L. Emig +4

Context. The combined use of carbon radio recombination lines (CRRLs) and the 158 m-[CII] line is a powerful tool for the study of the energetics and physical conditions (e.g.,…

astro-ph.HE2019

Are starburst galaxies a common source of high energy neutrinos and cosmic rays?

Cecilia Lunardini, Gregory S. Vance, Kimberly L. Emig +1

A recent analysis of cosmic ray air showers observed at the Pierre Auger Observatory indicates that nearby starburst galaxies (SBGs) might be the cause of ~10% of the Ultra-High-En…

astro-ph.GA2018

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

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.GA201725 cited

LOFAR observations of decameter carbon radio recombination lines towards Cassiopeia A

P. Salas, J. B. R. Oonk, R. J. van Weeren +6

We present a study of carbon radio recombination lines towards Cassiopeia A using LOFAR observations in the frequency range 10-33 MHz. Individual carbon lines are detected in a…