Pedro I. T. K. Sarmento
IA

Abstract
Gaia is a very powerful tool that can and will be used to detect exoplanets (Jordi et al. 2010; Martin-Fleitas et al. 2014; Sahlmann et al. 2014; Casertano et al. 2008; Perryman et al. 2014), with astrometry and radial velocity methods as well. In this Cookie Seminar, three important factors related to that will be analyzed: the planet detection threshold, the astrometry movements by the stars (that can indicate the presence of planets) and the construction of a database of bright stars as observed from earth, to use as a potential star sample for exoplanet research. Additionally, some results obtained with the database and current population of stars observed with the different methods for exoplanet detection will be explored.

09 December 2015, 13:30

Centro de Astrofísica
Rua das Estrelas
4150-762 Porto