activity
20142022
most citedA large light-mass component of cosmic rays at 10^{17} - 10^{17.5} eV from radio observations

156 citations · 854 across the 30 of their papers we have counts for

collaborators
Showing 2015Show all

8 papers · 1 filter

astro-ph.HE2015★ 7 cited

Orbital and superorbital variability of LS I +61 303 at low radio frequencies with GMRT and LOFAR

B. Marcote, M. Ribó, J. M. Paredes +23

LS I +61 303 is a gamma-ray binary that exhibits an outburst at GHz frequencies each orbital cycle of 26.5 d and a superorbital modulation with a period of 4.6…

astro-ph.HE2015★ 71 cited

LOFAR MSSS: Detection of a low-frequency radio transient in 400 hrs of monitoring of the North Celestial Pole

A. J. Stewart, R. P. Fender, J. W. Broderick +99

We present the results of a four-month campaign searching for low-frequency radio transients near the North Celestial Pole with the Low-Frequency Array (LOFAR), as part of the Mult…

astro-ph.IM2015★ 52 cited

The ASKAP/EMU Source Finding Data Challenge

A. M. Hopkins, M. T. Whiting, N. Seymour +31

The Evolutionary Map of the Universe (EMU) is a proposed radio continuum survey of the Southern Hemisphere up to declination +30 deg., with the Australian Square Kilometre Array Pa…

astro-ph.IM2015★ 105 cited

The LOFAR Multifrequency Snapshot Sky Survey (MSSS) I. Survey description and first results

G. H. Heald, R. F. Pizzo, E. Orrú +147

We present the Multifrequency Snapshot Sky Survey (MSSS), the first northern-sky LOFAR imaging survey. In this introductory paper, we first describe in detail the motivation and de…

astro-ph.IM2015★ 58 cited

Calibrating the absolute amplitude scale for air showers measured at LOFAR

A. Nelles, J. R. Hörandel, T. Karskens +74

Air showers induced by cosmic rays create nanosecond pulses detectable at radio frequencies. These pulses have been measured successfully in the past few years at the LOw Frequency…

astro-ph.SR2015

LOFAR discovery of a quiet emission mode in PSR B0823+26

C. Sobey, N. J. Young, J. W. T. Hessels +91

PSR B0823+26, a 0.53-s radio pulsar, displays a host of emission phenomena over timescales of seconds to (at least) hours, including nulling, subpulse drifting, and mode-changing.…