F
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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Journal ArticleDOI
Elodie metallicity-biased search for transiting Hot Jupiters I. Two Hot Jupiters orbiting the slightly evolved stars HD118203 and HD149143
R. F. Da Silva,Stéphane Udry,François Bouchy,M. Mayor,C. Moutou,Frederic Pont,D. Queloz,N. C. Santos,D. Segransan,Shay Zucker +9 more
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.
Journal ArticleDOI
KOI-200 b and KOI-889 b: Two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N
Guillaume Hébrard,Guillaume Hébrard,J. M. Almenara,Alexandre Santerne,Alexandre Santerne,Magali Deleuil,Cilia Damiani,Aldo S. Bonomo,Aldo S. Bonomo,François Bouchy,G. Bruno,Rodrigo F. Díaz,G. Montagnier,G. Montagnier,C. Moutou +14 more
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.
Journal ArticleDOI
Solar-like oscillations in the metal-poor subgiant nu Indi: constraining the mass and age using asteroseismology
Timothy R. Bedding,R. Paul Butler,Fabien Carrier,François Bouchy,Brendon J. Brewer,Patrick Eggenberger,Frank Grundahl,Hans Kjeldsen,Chris McCarthy,Tine Nielsen,A. Retter,C. G. Tinney +11 more
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.
Journal ArticleDOI
ESPRESSO high resolution transmission spectroscopy of WASP-76b.
Hugo M. Tabernero,M. R. Zapatero Osorio,Romain Allart,Francesco Borsa,Núria Casasayas-Barris,O. D. S. Demangeon,David Ehrenreich,J. Lillo-Box,C. Lovis,Enric Palle,S. G. Sousa,Rafael Rebolo,N. C. Santos,Francesco Pepe,S. Cristiani,Vardan Adibekyan,C. Allende Prieto,Yann Alibert,S. C. C. Barros,François Bouchy,Vincent Bourrier,Valentina D'Odorico,Xavier Dumusque,J. P. Faria,P. Figueira,R. Génova Santos,J. I. González Hernández,S. Hojjatpanah,G. Lo Curto,Baptiste Lavie,Cristina Martins,J. H. C. Martins,Andrea Mehner,Giuseppina Micela,Paolo Molaro,Nelson J. Nunes,E. Poretti,Julia V. Seidel,Alessandro Sozzetti,A. Suárez Mascareño,Stéphane Udry,Matteo Aliverti,M. Affolter,Diogo Alves,M. Amate,G. Avila,T. Bandy,Willy Benz,Antonino Bianco,C. Broeg,A. Cabral,Paolo Conconi,João Coelho,Claudio Cumani,S. Deiries,Hans Dekker,B. Delabre,A. Fragoso,Matteo Genoni,L. Genolet,I. Hughes,J. Knudstrup,F. Kerber,Marco Landoni,J. L. Lizon,C. Maire,Antonio Manescau,P. Di Marcantonio,Denis Mégevand,Mário J. P. F. G. Monteiro,M. Moschetti,E. Mueller,Andrea Modigliani,Luca Oggioni,Antonio Gouveia Oliveira,Giorgio Pariani,Luca Pasquini,Jose Luis Rasilla,Edoardo Maria Alberto Redaelli,Marco Riva,S. Santana-Tschudi,Paolo Santin,Pedro Santos,A. Segovia,D. Sosnowska,P. Spanò,F. Tenegi,Olaf Iwert,Alessio Zanutta,F. M. Zerbi +89 more
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.
Journal ArticleDOI
A precise architecture characterization of the $\pi$ Men planetary system
Mario Damasso,Alessandro Sozzetti,C. Lovis,S. C. C. Barros,S. G. Sousa,O. D. S. Demangeon,J. P. Faria,J. Lillo-Box,S. Cristiani,Francesco Pepe,Rafael Rebolo,N. C. Santos,M. R. Zapatero Osorio,J. I. González Hernández,M. Amate,Luca Pasquini,F. M. Zerbi,Vardan Adibekyan,Manuel Abreu,M. Affolter,Yann Alibert,Matteo Aliverti,Romain Allart,C. Allende Prieto,D. Álvarez,Diogo Alves,G. Avila,V. Baldini,T. Bandy,Willy Benz,Antonino Bianco,Francesco Borsa,Diego Bossini,Vincent Bourrier,François Bouchy,C. Broeg,A. Cabral,G. Calderone,Roberto Cirami,João Coelho,Paolo Conconi,Igor Coretti,Claudio Cumani,G. Cupani,Valentina D'Odorico,S. Deiries,Hans Dekker,B. Delabre,P. Di Marcantonio,Xavier Dumusque,David Ehrenreich,P. Figueira,A. Fragoso,L. Genolet,Matteo Genoni,R. Génova Santos,I. Hughes,Olaf Iwert,F. Kerber,J. Knudstrup,Marco Landoni,B. Lavie,J. L. Lizon,G. Lo Curto,C. Maire,Cristina Martins,Denis Mégevand,Andrea Mehner,Giuseppina Micela,Andrea Modigliani,Paolo Molaro,M. A. Monteiro,Mário J. P. F. G. Monteiro,M. Moschetti,E. Mueller,Michael T. Murphy,Nelson J. Nunes,Luca Oggioni,Antonio Gouveia Oliveira,Mahmoudreza Oshagh,Enric Palle,Giorgio Pariani,E. Poretti,Jose Luis Rasilla,José Manuel Rebordão,E. M. Redaelli,Marco Riva,S. Santana Tschudi,Paolo Santin,Pedro Santos,D. Segransan,T. M. Schmidt,A. Segovia,D. Sosnowska,P. Spanò,A. Suárez Mascareño,Hugo M. Tabernero,F. Tenegi,Stéphane Udry,Alessio Zanutta +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.