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Dive into the research topics where F. Thévenin is active.

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Featured researches published by F. Thévenin.


Astronomy and Astrophysics | 2004

The angular sizes of dwarf stars and subgiants Surface brightness relations calibrated by interferometry

P. Kervella; F. Thévenin; E. Di Folco; D. Ségransan

The availability of a number of new interferometric measurements of Main Sequence and subgiant stars makes it possible to calibrate the surface brightness relations of these stars using exclusively direct angular diameter measurements. These empirical laws make it possible to predict the limb darkened angular diameters


Astronomy and Astrophysics | 2003

The diameters of α Centauri A and B - A comparison of the asteroseismic and VINCI/VLTI views

Pierre Kervella; F. Thévenin; D. Ségransan; G. Berthomieu; B. Lopez; P. Morel; J. Provost

\theta_{\rm LD}


Astronomy and Astrophysics | 2004

VLTI near-IR interferometric observations of Vega-like stars: Radius and age of a PsA, b Leo, b Pic, e Eri and t Cet

E. Di Folco; F. Thévenin; Pierre Kervella; A. Domiciano de Souza; V. Coudé du Foresto; D. Ségransan; P. Morel

of dwarfs and subgiants using their dereddened Johnson magnitudes, or their effective temperature. The smallest intrinsic dispersions of


Astronomy and Astrophysics | 2007

A near-infrared interferometric survey of debris disk stars. I. Probing the hot dust content around eps Eridani and tau Ceti with CHARA/FLUOR

E. Di Folco; Olivier Absil; J.-C. Augereau; A. Mérand; V. Coudé du Foresto; F. Thévenin; Denis Defrere; P. Kervella; Theo A. ten Brummelaar; H. McAlister; Stephen T. Ridgway; J. Sturmann; L. Sturmann; Nils H. Turner

\sigma \le 1\%


The Astronomy and Astrophysics Review | 2007

Asteroseismology and interferometry

M. S. Cunha; Conny Aerts; Jørgen Christensen-Dalsgaard; A. Baglin; Lionel Bigot; Timothy M. Brown; C. Catala; O. L. Creevey; A. Domiciano de Souza; P. Eggenberger; Paulo Garcia; F. Grundahl; Pierre Kervella; D. W. Kurtz; P. Mathias; A. Miglio; M. J. P. F. G. Monteiro; G. Perrin; Frank Peter Pijpers; Dimitri Pourbaix; A. Quirrenbach; Karine Rousselet-Perraut; Teresa C. Teixeira; F. Thévenin; M. J. Thompson

in


Astronomy and Astrophysics | 2015

Gaia FGK benchmark stars: Effective temperatures and surface gravities

Ulrike Heiter; P. Jofre; Bengt Gustafsson; A. Korn; C. Soubiran; F. Thévenin

\theta_{\rm LD}


Astronomy and Astrophysics | 2002

Asteroseismology and calibration of alpha cen binary system

F. Thévenin; J. Provost; P. Morel; G. Berthomieu; Francois Bouchy; Fabien Carrier

are obtained for the relations based on the K and L magnitudes, for instance


Astronomy and Astrophysics | 2013

The Gaia astrophysical parameters inference system (Apsis) - Pre-launch description

Coryn A. L. Bailer-Jones; R. Andrae; Bernardino Arcay; T. L. Astraatmadja; I. Bellas-Velidis; A. Berihuete; A. Bijaoui; Claire Carrion; Carlos Dafonte; Y. Damerdji; A. Dapergolas; P. de Laverny; L. Delchambre; P. Drazinos; R. Drimmel; Y. Frémat; Diego Fustes; M. García-Torres; C. Guede; Ulrike Heiter; A.-M. Janotto; A. Karampelas; Dae-Won Kim; Jens Knude; I. Kolka; E. Kontizas; M. Kontizas; A. Korn; Alessandro C. Lanzafame; Yveline Lebreton

\log \theta_{\rm LD} = 0.0502\,(B-L) + 0.5133 - 0.2\,L


Monthly Notices of the Royal Astronomical Society | 2005

Spectroscopic survey of the Galaxy with Gaia– II. The expected science yield from the Radial Velocity Spectrometer

M. I. Wilkinson; A. Vallenari; C. Turon; Ulisse Munari; Daniel Martin Katz; G. Bono; Mark Cropper; Amina Helmi; N. Robichon; F. Thévenin; S. Vidrih; T. Zwitter; F. Arenou; M.-O. Baylac; G. Bertelli; A. Bijaoui; F. Boschi; F. Castelli; F. Crifo; M. David; Andreja Gomboc; Alfredo Gomez; M. Haywood; U. Jauregi; P. de Laverny; Y. Lebreton; P. M. Marrese; T. R. Marsh; S. Mignot; D. Morin

or


Astronomy and Astrophysics | 2014

On the fine structure of the Cepheid metallicity gradient in the Galactic thin disk

K. Genovali; B. Lemasle; G. Bono; M. Romaniello; M. Fabrizio; I. Ferraro; G. Iannicola; C. D. Laney; M. Nonino; Maria Bergemann; R. Buonanno; P. François; L. Inno; R.-P. Kudritzki; Noriyuki Matsunaga; S. Pedicelli; F. Primas; F. Thévenin

\log \theta_{\rm LD} = 0.0755\,(V-K) + 0.5170 - 0.2\rm \,K

Collaboration


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P. Morel

University of Nice Sophia Antipolis

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G. Bono

Sapienza University of Rome

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G. Jasniewicz

University of Montpellier

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J. Provost

Centre national de la recherche scientifique

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Thibault Merle

Université libre de Bruxelles

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G. Berthomieu

Centre national de la recherche scientifique

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