Iker Millán-Irigoyen
CIEMAT-FP, Madrid

Abstract
We are going to present the newly developed tools of stellar population synthesis code, pyPOPSTAR, and FADO galaxy spectral analysis code. In order to test the limits the all the new tool that we have developed, we are going to use the future VLT/MOONS instrument to see how the our tools reconstruct the properties of high redshift galaxies, such as the star formation history, the metallicity evolution history, the age of the galaxy,...

2020 January 31, 13:30

IA/U.Porto
Centro de Astrofísica da Universidade do Porto (Auditorium)
Rua das Estrelas, 4150-762 Porto