activity
20142026
most citedTwo planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf

114 citations · 523 across the 31 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2026

The attempted polarity reversal and evolving magnetic environment of AD Leo

K. G. Smith, D. Evensberget, S. Bellotti +3

In the past two decades, the observed large-scale magnetic field of the active M dwarf star AD Leo has evolved from strongly to mildly negative, raising a suspicion that it might s…

astro-ph.SR2025

Spectropolarimetric characterisation of exoplanet host stars in preparation of the mission II. The magnetised wind environment of TOI-1860, DS Tuc A, and HD 63433

S. Bellotti, A. Lavail, D. Evensberget +10

We update the status of the spectropolarimetric campaign dedicated to characterise the magnetic field properties of a sample of known exoplanet-hosting stars included in the curren…

astro-ph.SR2025★ 1 cited

A magnetic field study of two fast-rotating, radio bright M dwarfs. StKM 1-1262 and V374 Peg

S. Bellotti, P. I. Cristofari, J. R. Callingham +8

Radio observations at low frequencies are sensitive to the magnetic activity of stars and the plasma environment surrounding them. The accurate interpretation of the processes unde…

astro-ph.EP2025★ 3 cited

Characterizing planetary systems with SPIRou: Detection of a sub-Neptune in a 6-day period orbit around the M dwarf Gl 410

A. Carmona, X. Delfosse, M. Ould-Elhkim +42

The search for exoplanets around nearby M dwarfs represents a crucial milestone in the census of planetary systems in the vicinity of our Solar System. Since 2018 our team is carry…

astro-ph.SR2024★ 13 cited

A BCool survey of stellar magnetic cycles

S. Bellotti, P. Petit, S. V. Jeffers +6

The magnetic cycle on the Sun consists of two consecutive 11-yr sunspot cycles and exhibits a polarity reversal around sunspot maximum. Although solar dynamo theories have progress…

astro-ph.EP2024

Radio Signatures of Star-Planet Interactions, Exoplanets, and Space Weather

J. R. Callingham, B. J. S. Pope, R. D. Kavanagh +22

Radio detections of stellar systems provide a window onto stellar magnetic activity and the space weather conditions of extrasolar planets, information that is difficult to attain…

astro-ph.IM2024★ 2 cited

ANDES, the high resolution spectrograph for the ELT: science goals, project overview and future developments

A. Marconi, M. Abreu, V. Adibekyan +286

The first generation of ELT instruments includes an optical-infrared high-resolution spectrograph, indicated as ELT-HIRES and recently christened ANDES (ArmazoNes high Dispersion E…

astro-ph.EP2024

Spectropolarimetric characterisation of exoplanet host stars in preparation of the Ariel mission. Magnetic environment of HD 63433

S. Bellotti, D. Evensberget, A. A. Vidotto +8

The accurate characterisation of the stellar magnetism of planetary host stars has been gaining momentum, especially in the context of transmission spectroscopy investigations of e…

astro-ph.SR2024

Long-term monitoring of large-scale magnetic fields across optical and near-infrared domains with ESPaDOnS, Narval and SPIRou. The cases of EV Lac, DS Leo, and CN Leo

S. Bellotti, J. Morin, L. T. Lehmann +18

Dynamo models of stellar magnetic fields for partly and fully convective stars are guided by observational constraints. Zeeman-Doppler imaging has revealed a variety of magnetic fi…

astro-ph.SR2023

A long-term study of the magnetic field and activity in the M giant RZ Ari

R. Konstantinova-Antova, S. Georgiev, A. Lèbre +12

We present a detailed long-term study of the single M6 III giant RZ~Ari to obtain direct and simultaneous measurements of the magnetic field, activity indicators, and radial veloci…

astro-ph.SR2023

The large-scale magnetic field of the M dwarf double-line spectroscopic binary FK Aqr

S. Tsvetkova, J. Morin, C. P. Folsom +10

This work is part of the BinaMIcS project, the aim of which is to understand the interaction between binarity and magnetism in close binary systems. All the studied spectroscopic b…

astro-ph.SR2023

SPIRou reveals unusually strong magnetic fields of slowly rotating M dwarfs

L. T. Lehmann, J. -F. Donati, P. Fouque +8

In this paper, we study six slowly rotating mid-to-late M~dwarfs (rotation period ) by analysing spectropolarimetric data collected wi…

astro-ph.SR2023★ 7 cited

Correlations between laboratory line lists for FeH, CrH, and NiH and M-star spectra collected with ESPaDOnS and SPIRou

P. Crozet, J. Morin, A. J. Ross +9

Molecular bands of metal oxides and hydrides dominate the optical and near-infrared spectra of M dwarfs. High-resolution spectra of these bands have immense potential for determini…

astro-ph.SR2023★ 25 cited

The space weather around the exoplanet GJ 436 b. II. Stellar wind-exoplanet interactions

A. A. Vidotto, V. Bourrier, R. Fares +5

The M dwarf star GJ 436 hosts a warm-Neptune that is losing substantial amount of atmosphere, which is then shaped by the interactions with the wind of the host star. The stellar w…

astro-ph.SR2023

Magnetic fields & rotation periods of M dwarfs from SPIRou spectra

J. -F. Donati, L. T. Lehmann, P. I. Cristofari +17

We present near-infrared spectropolarimetric observations of a sample of 43 weakly- to moderately-active M dwarfs, carried with SPIRou at the Canada-France-Hawaii Telescope in the…

astro-ph.EP2023★ 1 cited

Characterizing planetary systems with SPIRou: M-dwarf planet-search survey and the multiplanet systems GJ 876 and GJ 1148

C. Moutou, X. Delfosse, A. C. Petit +18

SPIRou is a near-infrared spectropolarimeter and a high-precision velocimeter. The SPIRou Legacy Survey collected data from February 2019 to June 2022, half of the time devoted to…

astro-ph.SR2023★ 35 cited

Monitoring the large-scale magnetic field of AD~Leo with SPIRou, ESPaDOnS and Narval. Toward a magnetic polarity reversal?

S. Bellotti, J. Morin, L. T. Lehmann +23

One manifestation of dynamo action on the Sun is the 22-yr magnetic cycle, exhibiting a polarity reversal and a periodic conversion between poloidal and toroidal fields. For M dwar…

astro-ph.SR2023★ 21 cited

The space weather around the exoplanet GJ 436b

S. Bellotti, R. Fares, A. A. Vidotto +7

The space environment in which planets are embedded depends mainly on the host star and impacts the evolution of the planetary atmosphere. The quiet M dwarf GJ 436 hosts a close-in…

astro-ph.SR2023★ 79 cited

The magnetic field and multiple planets of the young dwarf AU~Mic

J. -F. Donati, P. I. Cristofari, B. Finociety +25

In this paper we present an analysis of near-infrared spectropolarimetric and velocimetric data of the young M dwarf AU Mic, collected with SPIRou at the Canada-France-Hawaii teles…

astro-ph.SR2023

Near-IR and optical radial velocities of the active M dwarf star Gl 388 (AD Leo) with SPIRou at CFHT and SOPHIE at OHP: A 2.23 day rotation period and no evidence for a corotating planet

A. Carmona, X. Delfosse, S. Bellotti +36

Context: The search for extrasolar planets around the nearest M dwarfs is a crucial step towards identifying the nearest Earth-like planets. One of the main challenges in this sear…

astro-ph.SR2023★ 21 cited

Optical and near-infrared stellar activity characterization of the early M dwarf Gl~205 with SOPHIE and SPIRou

P. Cortes-Zuleta, I. Boisse, B. Klein +41

The stellar activity of M dwarfs is the main limitation for discovering and characterizing exoplanets orbiting them since it induces quasi-periodic RV variations. We aim to charact…

astro-ph.SR2023★ 37 cited

The SPIRou Legacy Survey Rotation period of quiet M dwarfs from circular polarization in near-infrared spectral lines: I. The SPIRou APERO analysis

P. Fouqué, E. Martioli, J. -F. Donati +21

Context. The rotation period of stars is an important parameter along with mass, radius, effective temperature. It is an essential parameter for any radial velocity monitoring, as…

astro-ph.SR2023★ 10 cited

Misalignment of the outer disk of DK Tau and a first look at its magnetic field using spectropolarimetry

M. Nelissen, P. McGinnis, C. P. Folsom +7

Misalignments between a forming star's rotation axis and its outer disk axis, although not predicted by standard theories of stellar formation, have been observed in several classi…

astro-ph.SR2022★ 7 cited

Can scallop-shell stars trap dust in their magnetic fields?

Hannah Sanderson, Moira Jardine, Andrew Collier Cameron +2

One of the puzzles to have emerged from the Kepler and TESS missions is the existence of unexplained dips in the lightcurves of a small fraction of rapidly-rotating M dwarfs in you…