Context. Gravito-inertial asteroseismology came into existence thanks to high-precision
CoRoT and Kepler space photometric light curves. So far, it has given rise to the internal …

We present orbital elements, orbital parallaxes, and individual component masses for 14
spatially resolved double-line spectroscopic binaries derived doing a simultaneous fit of …

We present a Bayesian inference methodology for the estimation of orbital parameters on
single-line spectroscopic binaries with astrometric data, based on the No-U-Turn sampler …

We present results from Speckle inteferometric observations of 15 visual binaries and one
double-line spectroscopic binary, carried out with the HRCam Speckle camera of the SOAR …

Estimates of orbital parameters were made using a Bayesian optimization technique on
astrometric data for 25 visual binary systems catalogued a century ago by the ninth …

Mass is the fundamental parameter that determines the structure and evolution of a star.
Measuring the masses of the stars is however not an easy task, so the number of stars with …

Determining stellar masses remains a fundamental challenge in astrophysics, and binary
star systems offer a unique opportunity to measure these masses directly using Kepler's …

We present a Bayesian inference methodology for the estimation of orbital parameters on
single-line spectroscopic binaries with astrometric data, based on the No-U-Turn sampler …

Under certain rather prevalent conditions (driven by dynamical orbital evolution), a
hierarchical triple stellar system can be well approximated, from the standpoint of orbital …

We describe an ecosystem for teaching data science (DS) to engineers that blends theory,
methods, and applications, developed at the Faculty of Physical and Mathematical Sciences …