activity
20082025
most citedA multi-site campaign to measure solar-like oscillations in Procyon. I. Observations, Data Reduction and Slow Variations

158 citations · 397 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2025★ 11 cited

Helioseismic inference of the solar radiative opacity

Gaël Buldgen, Jean-Christophe Pain, Philippe Cossé +18

The Sun is the most studied of all stars, and thus constitutes a benchmark for stellar models. However, our vision of the Sun is still incomplete, as illustrated by the current deb…

astro-ph.SR2024

In-depth analysis of solar models with high-metallicity abundances and updated opacity tables

G. Buldgen, A. Noels, R. Scuflaire +10

Due to the high quality constraints available for the Sun, we can carry out combined analyses using neutrino, spectroscopic and helioseismic observations. Such studies lay the grou…

astro-ph.SR2019

From the Sun to solar-like stars: how does the solar modelling problem affect our studies of solar-like oscillators?

G. Buldgen, C. Pezzotti, M. Farnir +2

Since the first observations of solar oscillations in 1962, helioseismology has probably been one of the most successful fields of astrophysics. Besides the improvement of observat…

astro-ph.SR2018★ 40 cited

Mean density inversions for red giants and red clump stars

Gaël Buldgen, B. Rendle, T. Sonoi +8

Since the CoRoT and Kepler missions, the availability of high quality seismic spectra for red giants has made them the standard clocks and rulers for Galactic Archeology. With the…

astro-ph.SR2017★ 22 cited

Seismic inversion of the solar entropy: A case for improving the Standard Solar Model

G. Buldgen, S. J. A. J. Salmon, A. Noels +9

The Sun is the most constrained and well-studied of all stars. As a consequence, the physical ingredients entering solar models are used as a reference to study all other stars obs…

astro-ph.SR2010★ 3 cited

Asteroseismology of Solar-type stars with Kepler II: Stellar Modeling

T. S. Metcalfe, M. J. P. F. G. Monteiro, M. J. Thompson +9

Observations from the Kepler satellite were recently published for three bright G-type stars, which were monitored during the first 33.5d of science operations. One of these stars,…

astro-ph.SR2010★ 9 cited

Asteroseismology of Solar-type Stars with Kepler I: Data Analysis

C. Karoff, W. J. Chaplin, T. Appourchaux +46

We report on the first asteroseismic analysis of solar-type stars observed by Kepler. Observations of three G-type stars, made at one-minute cadence during the first 33.5d of scien…

astro-ph.SR2010★ 154 cited

The asteroseismic potential of Kepler: first results for solar-type stars

W. J. Chaplin, T. Appourchaux, Y. Elsworth +105

We present preliminary asteroseismic results from Kepler on three G-type stars. The observations, made at one-minute cadence during the first 33.5d of science operations, reveal hi…

astro-ph2008★ 158 cited

A multi-site campaign to measure solar-like oscillations in Procyon. I. Observations, Data Reduction and Slow Variations

Torben Arentoft, Hans Kjeldsen, Timothy R. Bedding +45

We have carried out a multi-site campaign to measure oscillations in the F5 star Procyon A. We obtained high-precision velocity observations over more than three weeks with eleven…