Yearslong time series of high-precision brightness measurements have been assembled for
thousands of stars with telescopes operating in space. Such data have allowed astronomers …

Oscillations detected on the solar surface provide a unique opportunity for investigations of
the interior properties of a star. Through major observational efforts, including extensive …

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 …

We compute a new generation of standard solar models (SSMs) that includes recent
updates on some important nuclear reaction rates and a more consistent treatment of the …

We present the updated version of the code used to compute stellar evolutionary tracks in
Padova. It is the result of a thorough revision of the major input physics, together with the …

Our understanding of the properties and demographics of exoplanets critically relies on our
ability to determine the fundamental properties of their host stars. The advent of Gaia and …