activity
20032010
most citedA multi-site campaign to measure solar-like oscillations in Procyon. I. Observations, Data Reduction and Slow Variations

158 citations · 547 across the 10 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 3 cited

The seismology programme of CoRoT

E. Michel, A. Baglin, M. Auvergne +1

We introduce the main lines and specificities of the CoRoT Seismology Core Programme. The development and consolidation of this programme has been made in the framework of the CoRo…

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…

astro-ph2008★ 79 cited

Sensitivity of helioseismic gravity modes to the dynamics of the solar core

S. Mathur, A. Eff-Darwich, R. A. García +1

The dynamics of the solar core cannot be properly constrained through the analysis of acoustic oscillation modes. Gravity modes are necessary to understand the structure and dynami…

astro-ph2006★ 9 cited

Curvelet analysis of asteroseismic data I: Method description and application to simulated sun-like stars

P. Lambert, S. Pires, J. Ballot +3

Context: The detection and identification of oscillation modes (in terms of their , and successive ) is a great challenge for present and future asteroseismic space mi…

astro-ph2004★ 157 cited

Surprising Sun

S. Turck-Chieze, S. Couvidat, L. Piau +5

Important revisions of the solar model ingredients appear after 35 years of intense work which have led to an excellent agreement between solar models and solar neutrino detections…

astro-ph2003★ 132 cited

The Rotation Of The Deep Solar Layers

S. Couvidat, R. A. Garcia, S. Turck-Chieze +3

From the analysis of low-order GOLF+MDI sectoral modes and LOWL data (l > 3), we derive the solar radial rotation profile assuming no latitudinal dependance in the solar core. Thes…