Caracterización de la rotación en surveys fotométricos: Preparación para TESS (NASA) y PLATO (ESA)

Abstract

With this project we had two goals. The first one is to get familiarized with asteroseismology techniques to precisely determine masses and radii of stars. The second goal is to study the surface rotation of numerical simulations of the PLATO mission and of real degraded data obtained by the Kepler mission to simulate the observation conditions of the TESS and PLATO missions. By analyzing these data, we want to find the limits of the current methods used to determine surface rotation from light curves and evaluate the reliability and completeness of the results.