Supervisors: José Antonio Caballero Hernández, Jorge Sanz Forcada
BSc/Licenciate Degree in Physics in Universidad de Salamanca, and MSc in Astrophysics in Universidad Complutense de Madrid.
Since 2017 investigates, inside the CARMENES consortium, the properties of M dwarfs, which are the most common type of stars in the Galaxy.
CARMENES was conceived as an instrument and as a project to discover rocky, temperate, Earth-like planets in the habitable zones of M dwarfs.
GitHub: https://github.com/ccifuentesr
| Keywords | Cool stars — Low-mass stars — Exoplanets — Photometry — Stellar catalogues |
