activity
20082026
most citedThe Giant Radio Array for Neutrino Detection (GRAND): Science and Design

293 citations · 888 across the 24 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

6 papers · 1 filter

astro-ph.SR2026

Probing the magnetic field of a coronal mass ejection with PSR J1022+1001

El Mehdi Zahraoui, Hannah T. Rüdisser, Golam M. Shaifullah +24

We investigate whether low-frequency pulsar observations can provide LoS magnetic field estimates and whether these are consistent with synthetic LoS signatures extracted from a th…

astro-ph.SR2025

Occurrence rate of stellar Type II radio bursts from a 100 star-year search for coronal mass ejections

David C. Konijn, Harish K. Vedantham, Cyril Tasse +8

Coronal mass ejections (CMEs) are major drivers of space weather in the Solar System, but their occurrence rate on other stars is unknown. A characteristic (deca-)metric radio burs…

astro-ph.SR2025

A predictive framework for realistic star planet radio emission in compact systems

J. J. Chebly, C. K. Louis, A. Strugarek +2

Radio emission from star planet interactions (SPI) beyond our solar system has yet to be firmly detected, primarily due to challenges such as weak signals, directional beaming effe…

astro-ph.SR2025★ 12 cited

Radio Burst from a Stellar Coronal Mass Ejection

J. R. Callingham, C. Tasse, R. Keers +15

Coronal mass ejections (CMEs) are massive expulsions of magnetised plasma from a star, and are the largest contributors to space weather in the Solar System. CMEs are theorized to…

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.…

astro-ph.SR2010★ 205 cited

Searching for Star-Planet interactions within the magnetosphere of HD 189733

R. Fares, J. -F. Donati, C. Moutou +7

HD 189733 is a K2 dwarf, orbited by a giant planet at 8.8 stellar radii. In order to study magnetospheric interactions between the star and the planet, we explore the large-scale m…