activity
19982026
most citedCARMENES input catalogue of M dwarfs: III. Rotation and activity from high-resolution spectroscopic observations

137 citations · 467 across the 25 of their papers we have counts for

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astro-ph.SR2026

Euclid: The convective-transition gap of 47 Tuc

M. Libralato, M. Griggio, R. Gerasimov +140

We report the first detection of the `convective-transition gap' (also known as `M-dwarf gap') in the globular cluster 47 Tuc (NGC 104) thanks to Euclid data. This feature, linked…

astro-ph.SR2026

The Variability of Radio Stars

Laura N. Driessen, Alex Andersson, Joseph R. Callingham +6

Stellar radio emission is highly variable with stellar flares lasting from milliseconds to hours. For some stars, their flares or bursts can repeat once every couple of hours, whil…

astro-ph.SR2019★ 6 cited

Science Requirement Document (SRD) for the European Solar Telescope (EST) (3rd Edition, December 2025)

Rolf Schlichenmaier, Luis R. Bellot Rubio, Manuel Collados Vera +31

The European Strategy Forum on Research Infrastructures (ESFRI) included the European Solar Telescope (EST) as an ESFRI Project in its 2016 Roadmap and confirmed this status in 202…

astro-ph.SR2018★ 110 cited

CARMENES input catalogue of M dwarfs IV. New rotation periods from photometric time series

E. Diez Alonso, J. A. Caballero, D. Montes +21

Aims. The main goal of this work is to measure rotation periods of the M-type dwarf stars being observed by the CARMENES exoplanet survey to help distinguish radial-velocity signal…

astro-ph.SR2018★ 137 cited

CARMENES input catalogue of M dwarfs: III. Rotation and activity from high-resolution spectroscopic observations

S. V. Jeffers, P. Schoefer, A. Lamert +18

CARMENES is a spectrograph for radial velocity surveys of M dwarfs with the aim of detecting Earth-mass planets orbiting in the habitable zones of their host stars. To ensure an op…

astro-ph.SR2015

Capella (alpha Aurigae) revisited: New binary orbit, physical properties, and evolutionary state

Guillermo Torres, Antonio Claret, Kresimir Pavlovski +1

Knowledge of the chemical composition and absolute masses of Capella are key to understanding the evolutionary state of this benchmark binary system comprising two giant stars. Pre…