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D. Salabert

Researcher at University of Nice Sophia Antipolis

Publications -  91
Citations -  5366

D. Salabert is an academic researcher from University of Nice Sophia Antipolis. The author has contributed to research in topics: Stars & Asteroseismology. The author has an hindex of 34, co-authored 87 publications receiving 5176 citations. Previous affiliations of D. Salabert include Centre national de la recherche scientifique & University of La Laguna.

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Asteroseismic fundamental properties of solar-type stars observed by the nasa kepler mission

TL;DR: In this article, a grid-based analysis was used to estimate the fundamental properties of more than 500 main-sequence and sub-giant stars using the NASA Kepler data obtained during the first 10 months of Kepler science operations, when these solar-type targets were observed for one month each in survey mode.
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Ensemble Asteroseismology of Solar-Type Stars with the NASA Kepler Mission

TL;DR: It is found that the distribution of observed masses of these stars shows intriguing differences to predictions from models of synthetic stellar populations in the Galaxy.
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Testing scaling relations for solar-like oscillations from the main sequence to red giants using kepler data

TL;DR: In this paper, the authors analyzed solar-like oscillations in ~1700 stars observed by the Kepler Mission, spanning from the main sequence to the red clump, and found that the difference of the Δν-νmax relation for unevolved and evolved stars can be explained by different distributions in effective temperature and stellar mass, in agreement with what is expected from scaling relations.
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Testing Scaling Relations for Solar-Like Oscillations from the Main Sequence to Red Giants using Kepler Data

TL;DR: In this paper, the authors analyzed solar-like oscillations in ~1700 stars observed by the Kepler Mission, spanning from the main-sequence to the red clump, and showed that the difference of the Delta-nu-nu -max relation for unevolved and evolved stars can be explained by different distributions in effective temperature and stellar mass, in agreement with what is expected from scaling relations.