activity
20162023
most citedRadial-Velocity Fitting Challenge. II. First results of the analysis of the data set

115 citations · 432 across the 8 of their papers we have counts for

collaborators

9 papers

astro-ph.EP20241 cited

TESS and ESPRESSO discover a super-Earth and a mini-Neptune orbiting the K-dwarf TOI-238

A. Suárez Mascareño, V. M. Passegger, J. I. González Hernández +53

The number of super-Earth and mini-Neptune planet discoveries has increased significantly in the last two decades thanks to transit and radial velocity surveys. When it is possible…

astro-ph.IM202343 cited

Statistical methods for exoplanet detection with radial velocities

Nathan C. Hara, Eric B. Ford

Exoplanets can be detected with various observational techniques. Among them, radial velocity (RV) has the key advantages of revealing the architecture of planetary systems and mea…

astro-ph.SR202321 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.EP202350 cited

Two temperate Earth-mass planets orbiting the nearby star GJ1002

A. Suárez Mascareño, E. González-Álvarez, M. R. Zapatero Osorio +42

We report the discovery and characterisation of two Earth-mass planets orbiting in the habitable zone of the nearby M-dwarf GJ~1002 based on the analysis of the radial-velocity (RV…

astro-ph.EP202373 cited

DREAM I. Orbital architecture orrery

V. Bourrier, O. Attia, M. Mallonn +28

The distribution of close-in exoplanets is shaped by a complex interplay between atmospheric and dynamical processes. The Desert-Rim Exoplanets Atmosphere and Migration (DREAM) pro…

astro-ph.EP202212 cited

A stellar occultation by the transneptunian object (50000) Quaoar observed by CHEOPS

B. E. Morgado, G. Bruno, A. R. Gomes-Júnior +82

Stellar occultation is a powerful technique that allows the determination of some physical parameters of the occulting object. The result depends on the photometric accuracy, the t…