We are entering a golden era for stellar physics driven by satellite and telescope
observations of unprecedented quality and scope. New insights on stellar evolution and …

Until the last few decades, investigations of stellar interiors had been restricted to theoretical
studies only constrained by observations of their global properties and external …

We present an updated release of the BaSTI (a Bag of Stellar Tracks and Isochrones) stellar
model and isochrone library for a solar-scaled heavy element distribution. The main input …

PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing
accurate key planet parameters (radius, mass, density and age) in statistical numbers, it …

We present a catalog of stellar properties for a large sample of 6676 evolved stars with
Apache Point Observatory Galactic Evolution Experiment spectroscopic parameters and …

We present a comparison of parallaxes and radii from asteroseismology and Gaia DR1
(TGAS) for 2200 Kepler stars spanning from the main sequence to the red-giant branch. We …

We present a study of 33 Kepler planet-candidate host stars for which asteroseismic
observations have sufficiently high signal-to-noise ratio to allow extraction of individual …

We use asteroseismic data from the Kepler satellite to determine fundamental stellar
properties of the 66 main-sequence targets observed for at least one full year by the mission …

The Kepler mission has provided exquisite data to perform an ensemble asteroseismic
analysis on evolved stars. In this work we systematically characterize solar-like oscillations …

Investigations of the origin and evolution of the Milky Way disc have long relied on chemical
and kinematic identifications of its components to reconstruct our Galactic past. Difficulties in …