activity
20162021
most citedThe LOFAR Tied-Array All-Sky Survey (LOTAAS): Survey overview and initial pulsar discoveries

106 citations · 228 across the 7 of their papers we have counts for

collaborators

17 papers

astro-ph.SR20211 cited

Observations of shock propagation through turbulent plasma in the solar corona

Eoin P. Carley, Baptiste Cecconi, Hamish A. Reid +14

Eruptive activity in the solar corona can often lead to the propagation of shock waves. In the radio domain the primary signature of such shocks are type II radio bursts, observed…

astro-ph.HE2021

Evidence of intra-binary shock emission from the redback pulsar PSR J1048+2339

A. Miraval Zanon, P. D'Avanzo, A. Ridolfi +16

We present simultaneous multiwavelength observations of the 4.66 ms redback pulsar PSR J1048+2339. We performed phase-resolved spectroscopy with the Very Large Telescope (VLT) sear…

astro-ph.SR20216 cited

LOFAR imaging of the solar corona during the 2015 March 20 solar eclipse

A. M. Ryan, P. T. Gallagher, E. P. Carley +12

The solar corona is a highly-structured plasma which can reach temperatures of more than ~2 MK. At low frequencies (decimetric and metric wavelengths), scattering and refraction of…

astro-ph.SR202125 cited

LOFAR observations of a jet-driven piston shock in the low solar corona

Ciara A. Maguire, Eoin P. Carley, Pietro Zucca +2

The Sun produces highly dynamic and eruptive events that can drive shocks through the corona. These shocks can accelerate electrons, which result in plasma emission in the form of…

astro-ph.HE202055 cited

The impact of Solar wind variability on pulsar timing

C. Tiburzi, G. M. Shaifullah, C. G. Bassa +22

High-precision pulsar timing requires accurate corrections for dispersive delays of radio waves, parametrized by the dispersion measure (DM), particularly if these delays are varia…

astro-ph.SR202013 cited

LOFAR observations of radio burst source sizes and scattering in the solar corona

Pearse C. Murphy, Eoin P. Carley, Aoife Maria Ryan +2

Low frequency radio wave scattering and refraction can have a dramatic effect on the observed size and position of radio sources in the solar corona. The scattering and refraction…