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

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

ESTALLIDOS includes experts in observational astrophysics, numerical simulations, theoretical modeling, and instrumentation. Working together on "star formation" for more than 20 years, we have played a leading role in the development of the field (> 1000 papers, > 30 PhD Theses). Our strength lies in the complementarity among the different

B-CycleS is born as an ambitious long-term research program that aims to provide a comprehensive picture for the formation and evolution of galaxies by studying the interplay between their two basic constituents: baryons and dark matter. B-CycleS is rooted in the detailed analysis of the stellar population properties of galaxies and equipped with

One of the main questions in Astrophysics is whether there are other Earths in the Galaxy. Our project is observational and technically prepared to address this question and lead to a significant progress on our understanding of the physical properties of planets, brown dwarfs, and stars, their formation mechanisms and evolution. We will conduct