Characterization of the Canary Island Observatories
The IAC has long been aware of the importance of promoting initiatives for the characterization and protection of the Canarian Observatories (Roque de los...
Stellar spectroscopy allows us to determine the properties and chemical compositions of stars. From this information for stars of different ages in the Milky...
CHromospheric magnetic fields in fLAREs and their evolution CHLARE
This project aims to study the variations of the solar magnetic field in flares, the most energetic events in our solar system. Flares accelerate charged...
Cosmic Evolution of Milky Way-like galaxies (CEMWAY)
In less than a decade, our understanding of the Milky Way has largely increased. It is now clear that we live in a disc-like galaxy hosting several stellar...
The Cosmic Microwave Background (CMB) contains the statistical information about the early seeds of the structure formation in our Universe. Its natural...
In addition to being a long-postulated particle that satisfactorily explains the absence of the neutron’s dipole moment observed in laboratories while...
EDUCADO: Exploring the Deep Universe by Computational Analysis of Data from Observations
The formation and evolution of massive galaxies is reasonably well understood in the context of the successful standard ΛCDM formalism. Such simulations of...
Galaxy evolution is a crucial topic in modern extragalactic astrophysics, linking cosmology to the Local Universe. Their study requires collecting statistically...