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François Bouchy

Researcher at Aix-Marseille University

Publications -  435
Citations -  30952

François Bouchy is an academic researcher from Aix-Marseille University. The author has contributed to research in topics: Planet & Exoplanet. The author has an hindex of 91, co-authored 417 publications receiving 29162 citations. Previous affiliations of François Bouchy include Pierre-and-Marie-Curie University & Centre national de la recherche scientifique.

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Elodie metallicity-biased search for transiting Hot Jupiters I. Two Hot Jupiters orbiting the slightly evolved stars HD118203 and HD149143

TL;DR: In this paper, the authors reported the discovery of a new planet candidate orbiting the subgiant star HD118203 with a period of P=6.1335 days and a minimum mass m2sin(i) = 2.1MJup.
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KOI-200 b and KOI-889 b: Two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N

TL;DR: In this article, the authors presented the detection and characterization of two new transiting, close-in, giant extrasolar planets KOI200 b and KOI-889 b, which were first identified by the Kepler team as promising candidates from photometry of the Kepler satellite, then established their planetary nature thanks to the radial velocity followup jointly secured with the spectrographs SOPHIE and HARPS-N.
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Solar-like oscillations in the metal-poor subgiant nu Indi: constraining the mass and age using asteroseismology

TL;DR: Asteroseismology is a powerful method for determining fundamental properties of stars as mentioned in this paper, which is the first application to a metal-poor object, namely the subgiant star nu Ind.
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ESPRESSO high resolution transmission spectroscopy of WASP-76b.

TL;DR: In this paper, high-resolution transmission spectroscopic observations of two primary transits of the highly-irradiated, ultra-hot Jupiter-size planet WASP-76b are reported.
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A precise architecture characterization of the $\pi$ Men planetary system

Mario Damasso, +99 more
TL;DR: In this article, the authors used the spectra of ESPRESSO for an independent determination of the stellar fundamental parameters and presented a precise characterization of the planetary system around the bright star $\pi$ Men.