The project focuses on the study of the effect of the internal structure of temperature and density in ionized nebulae on the determination of their chemical composition. The main objective is to carry out different independent verifications and analyze in depth the repercussions of our recent work published in Nature (Méndez-Delgado et al. 2023)

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

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

This grant funds the Development of DRAGO‑3 Payloads for Satellite Platforms project over a two‑year execution period (1 July 2025 – 1 July 2027). The IAC will design, validate and assemble eight DRAGO‑3 payloads optimised for operation within satellite constellations, covering the optical system, acquisition electronics, data processing and