scispace - formally typeset
F

Frédéric Baudin

Researcher at University of Paris-Sud

Publications -  137
Citations -  9020

Frédéric Baudin is an academic researcher from University of Paris-Sud. The author has contributed to research in topics: Stars & Asteroseismology. The author has an hindex of 52, co-authored 136 publications receiving 8565 citations. Previous affiliations of Frédéric Baudin include Centre national de la recherche scientifique & Université Paris-Saclay.

Papers
More filters
Journal ArticleDOI

The PLATO 2.0 mission

Heike Rauer, +167 more
TL;DR: The PLATO 2.0 mission as discussed by the authors has been selected for ESA's M3 launch opportunity (2022/24) to provide accurate key planet parameters (radius, mass, density and age) in statistical numbers.
Journal ArticleDOI

Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius

A. Léger, +162 more
TL;DR: In this paper, the authors reported the discovery of very shallow (ΔF/F ≈ 3.4× 10 −4 ) periodic dips in the light curve of an active V = 11.7 G9V star observed by the CoRoT satellite, which they interpret as caused by a transiting companion.
Journal ArticleDOI

Non-radial oscillation modes with long lifetimes in giant stars

TL;DR: The presence of radial and non-radial oscillations in more than 300 giant stars is reported, finding giant stars with equally spaced frequency peaks in the Fourier spectrum of the time series, as well as giants for which the spectrum seems to be more complex.
Journal ArticleDOI

The underlying physical meaning of the νmax νc relation

TL;DR: In this article, the authors provided a theoretical basis for the scaling between the frequency of the maximum in the power spectrum (νmax) of solar-like oscillations and the cut-off frequency (νc).
Journal ArticleDOI

Red-giant seismic properties analyzed with CoRoT

TL;DR: In this article, the authors performed an analysis of more than 4600 CoRoT light curves to extract as much information as possible, including the mean wide frequency separation of solar-like oscillations and the frequency of the maximum seismic amplitude, with the additional information of the effective temperature.