activity
20232026
most citedThe CARMENES search for exoplanets around M dwarfs. A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data

29 citations · 41 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2026

Discovering and Characterising Exoplanets and Ultracool Dwarfs with the Square Kilometre Array

Robert D. Kavanagh, Juan B. Climent, Philippe Zarka +14

The majority of the Solar System planets are sources of bright radio emission, driven by energetic electrons trapped within each planet's magnetic field. Detection of this emission…

astro-ph.EP2026★ 1 cited

Constraining an exoplanets magnetic field using star-planet interactions

D. Revilla, P. J. Amado, R. Luque +17

Theory predicts that a planet with a sufficiently strong magnetic field orbiting close to its host star could induce star-planet magnetic interactions. This is potentially observab…

astro-ph.SR2026

Searching for radio emission from stellar wind-magnetosphere interaction or co-rotation breakdown in brown dwarfs

Rebeca Pirvu Malanda, Simranpreet Kaur, Daniele Viganò +11

With the improvements in radio interferometry sensitivity, the quest for coherent radio emission from exoplanets and ultra-cool dwarfs, which is indicative of their magnetic fields…

astro-ph.SR2025★ 3 cited

Polarized, variable radio emission from the scallop-shell binary system DG CVn

Simranpreet Kaur, Daniele Viganò, Jackie Villadsen +9

DG CVn is an eruptive variable star and represents the closest member of the known sample of complex periodic variables, or scallop-shell stars. Over the years, this M dwarf binary…

astro-ph.EP2025

Rossby number regime, convection suppression, and dynamo-generated magnetism in inflated hot Jupiters

Albert Elias-López, Matteo Cantiello, Daniele Viganò +3

Hot Jupiters (HJs) are commonly thought to host the strongest dynamo-generated magnetic fields among exoplanets, up to one order of magnitude larger than Jupiter. Thus, they have o…

astro-ph.EP2025

First detection of variable radio emission originating from the infant planetary system V1298 Tau

M. Damasso, O. Morata, S. Kaur +13

V1298 Tau is a very young and magnetically active star which hosts a benchmark multi-planetary system to study planet formation and evolutionary history at the earliest stages. We…

astro-ph.SR2024★ 7 cited

Hints of auroral and magnetospheric polarized radio emission from the scallop-shell star 2MASS J050827292101444

Simranpreet Kaur, Daniele Viganò, Víctor J. S. Béjar +18

Scallop-shell stars, a recently discovered class of young M dwarfs, show complex optical light curves that are characterized by periodic dips as well as other features that are sta…

astro-ph.SR2024★ 1 cited

Variable, circularly polarized radio emission from the Young Stellar Object [BHB2007]-1: another ingredient of a unique system

Simranpreet Kaur, Josep M. Girart, Daniele Viganò +7

The young stellar object [BHB2007]-1 has been extensively studied in the past at radio, millimeter, and infrared wavelengths. It shows a gap in the disk and previous observations c…

astro-ph.EP2023★ 29 cited

The CARMENES search for exoplanets around M dwarfs. A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data

J. Blanco-Pozo, M. Perger, M. Damasso +37

Detecting a planetary companion in a short-period orbit through radio emission from the interaction with its host star is a new prospect in exoplanet science. Recently, a tantalisi…