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F. Thévenin

Researcher at Centre national de la recherche scientifique

Publications -  120
Citations -  25312

F. Thévenin is an academic researcher from Centre national de la recherche scientifique. The author has contributed to research in topics: Stars & Galaxy. The author has an hindex of 45, co-authored 113 publications receiving 20844 citations. Previous affiliations of F. Thévenin include University of Barcelona & University of Nice Sophia Antipolis.

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Gaia Data Release 3. Apsis. III. Non-stellar content and source classification

TL;DR: The contribution of the non-stellar and classification modules from the eighth coordination unit (CU8) of the Data Processing and Analysis Consortium, which is responsible for the determination of source astrophysical parameters using Gaia data, is presented in this paper .
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Oscillations in Procyon A First results from a multi-site campaign

TL;DR: In this paper, a spectroscopic multi-site campaign using 10 telescopes world-wide (minimizing aliasing effects) with a total time span of nearly 4 weeks (increase the frequency resolution) is performed to identify frequencies in this star and finally determine its properties and evolutionary state.
Posted Content

The limb darkening of αCentauri B Matching 3D hydrodynamical models with interferometric measurements

TL;DR: In this article, a 3D hydrodynamical radiative transfer model of the K1 V atmosphere was used to fit the new interferometric visibility measurements of α Cen B obtained with the VINCI instrument of the VLT Interferometer.
Journal ArticleDOI

On the accuracy of oscillator strengths in the near-infrared for the Gaia space mission

Lionel Bigot, +1 more
TL;DR: In this article, the authors tested the accuracy of oscillator strengths and wavelengths of some spectral lines (FeI, Si I, Ca II) of interest for the Gaia space mission in the near infrared (848-875 nm).
Journal Article

The Carina Dwarf Spheroidal Galaxy: A Goldmine for Cosmology and Stellar Astrophysics

TL;DR: In this paper, the Carina dwarf spheroidal galaxy has been analyzed using multiband (U, B, V, I) optical data collected using three different ground-based telescopes (4-metre Blanco CTIO, MPG/ESO 2.2metre, 1.5metre CTIO).