activity
20122020
most citedA hot Jupiter orbiting a 2-Myr-old solar-mass T Tauri star

150 citations · 752 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2020★ 50 cited

The large-scale magnetic field of Proxima Centauri near activity maximum

Baptiste Klein, Jean-François Donati, Élodie M. Hébrard +5

We report the detection of a large-scale magnetic field at the surface of the slowly-rotating fully-convective M dwarf Proxima Centauri. Ten circular polarization spectra, collecte…

astro-ph.SR2019★ 57 cited

Do non-dipolar magnetic fields contribute to spin-down torques?

Victor See, Sean P. Matt, Adam J. Finley +14

Main sequence low-mass stars are known to spin-down as a consequence of their magnetised stellar winds. However, estimating the precise rate of this spin-down is an open problem. T…

astro-ph.SR2019★ 93 cited

Estimating magnetic filling factors from Zeeman-Doppler magnetograms

Victor See, Sean P. Matt, Colin P. Folsom +15

Low-mass stars are known to have magnetic fields that are believed to be of dynamo origin. Two complementary techniques are principally used to characterise them. Zeeman-Doppler im…

astro-ph.EP2017★ 15 cited

Predictions of planet detections with near infrared radial velocities in the up-coming SPIRou Legacy Survey-Planet Search

Ryan Cloutier, Étienne Artigau, Xavier Delfosse +8

The SPIRou near infrared spectro-polarimeter is destined to begin science operations at the Canada-France-Hawaii Telescope in mid-2018. One of the instrument's primary science goal…

astro-ph.SR2017★ 71 cited

SPIRou Input Catalog: Activity, Rotation and Magnetic Field of Cool Dwarfs

C. Moutou, E. M. Hebrard, J. Morin +7

Based on optical high-resolution spectra obtained with CFHT/ESPaDOnS, we present new measurements of activity and magnetic field proxies of 442 low-mass K5-M7 dwarfs. The objects w…

astro-ph.SR2017★ 2 cited

A deep staring campaign in the Sigma Orionis cluster. Variability in substellar members

P. Elliott, A. Scholz, R. Jayawardhana +2

Deep optical imaging is used to study time-domain properties of young brown dwarfs in sigma Orionis over typical rotational time-scales and to search for new substellar and planeta…