57 citations · 182 across the 7 of their papers we have counts for
8 papers
Stellar masses and ages in Gaia Data Release 4 from the Final Luminosity Age Mass Estimator algorithm
Orlagh L. Creevey, Laia Casamiquela, Yveline Lebreton +23
The masses and ages of stars are key quantities for understanding exoplanetary, stellar, and galactic evolution. In the context of Gaia, these parameters provide insights into the…
On the seismic modelling of subgiant stars: testing different grid interpolation methods
Miguel Clara, Margarida S. Cunha, Pedro P. Avelino +3
Context. The emergence of mixed modes during the subgiant phase, whose frequencies are characterized by a fast evolution with age, can potentially enable a precise determination of…
Asteroseismic modelling strategies in the PLATO era. II. Automation of seismic inversions and quality assessment procedure
Jérôme Bétrisey, Gaël Buldgen, Daniel R. Reese +1
*Context*. In the framework of the PLATO mission, to be launched in late 2026, seismic inversion techniques will play a key role in the mission precision requirements of the stella…
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…
In-depth study of 16CygB using inversion techniques
G. Buldgen, S. J. A. S. Salmon, D. R. Reese +1
The 16Cyg binary system hosts the solar-like Kepler targets with the most stringent observational constraints. Moreover, this system is particularly interesting since both stars ar…
Using seismic inversions to obtain an internal mixing processes indicator for main-sequence solar-like stars
G. Buldgen, D. R. Reese, M. A. Dupret
Determining accurate and precise stellar ages is a major problem in astrophysics. These determinations are either obtained through empirical relations or model-dependent approaches…
Constraints on the structure of 16 Cyg A and 16 Cyg B using inversion techniques
G. Buldgen, D. R. Reese, M. A. Dupret
Constraining mixing processes and chemical composition is a central problem in stellar physics as their impact on stellar age determinations leads to biases in our studies of stell…
Estimating stellar mean density through seismic inversions
D. R. Reese, J. P. Marques, M. J. Goupil +2
Determining the mass of stars is crucial both to improving stellar evolution theory and to characterising exoplanetary systems. Asteroseismology offers a promising way to estimate…