The magnetic field is the main driver of the spectacular activity of the solar atmosphere, which covers the photosphere, chromosphere, transition region, and corona. This is true also for many other stars, although it is in the Suns atmosphere where we can observe the consequences of the interaction between an astrophysical plasma and its magnetic

The TANNHAUSER project is a public-private collaboration initiative in which the Instituto de Astrofísica de Canarias (IAC) participates as a collaborating partner. Its main objective is to develop and integrate an advanced optical communications system into the Nasmyth platform of the Two-meter Twin Telescope (TTT), located at the Teide

Black holes (BHs) are the pinnacle of extreme gravity. They are responsible for the most violent phenomena observed in the Universe, from long gamma-ray bursts, tidal disruption events to gravitational waves (GW). Despite the recent growth in extragalactic BH discoveries by LIGO-VIRGO, our knowledge of the seed BH population is severely hindered by

SUBSTELLAR project is aimed at mining the Euclid Telescope surveys for pushing the frontier of knowledge in substellar science. The first challenge of the project is to identify, based on Euclid data, an unprecedented large number (>1.000.000) of very low mass (VLM) stars and Substellar-mass Objects (SMOs), including hard to find objects such as

Las ayudas tienen como objeto la formación de doctores/as mediante la financiación de contratos laborales, bajo la modalidad de contrato predoctoral, a fin de que el personal investigador predoctoral en formación realice una tesis doctoral asociada a un proyecto de investigación financiado por las ayudas para proyectos de I+D del Subprograma

In this coordinated project, we propose to investigate fundamental questions concerning the formation and evolution of galaxies, by adopting the Galactic Archaeology approach. As the Sun is treated as a special star for the incredible amount of detail with which it can be studied, in the same way the Milky Way (MW) and Local Group (LG) galaxies are