This project is the natural continuation of the Coordinated Projects AYA2007-67752, AYA2010-21322 and AYA2013-48226 that were carried out by the Instituto de Astrofísica de Canarias (IAC), the Universidad Complutense de Madrid (UCM) and the Universitat de Valencia (UV). The fundamental objective of this proposal is to keep on deepening in our

Understanding the climate of our planet Earth is one of the greatest challenges in Science today. Much is still to be learned for example, on the variations of Earths albedo, or on external forcing factors, such as changes in the solar radiation. To truly go in depth into these open questions one may need to step out, view the Earth as a planet and

This research project aims to join efforts and consolidate the cooperation of a group of researchers with deep-rooted expertises and skills in different areas close or directly related to the AGN phenomenon, and with important national and international collaborations. We plan to make significant contributions to the resolution of some of the most

We propose to study the evolution of galaxies through detailed analysis of images and spectra obtained with the most modern ground- and space-based telescopes. We will concentrate on two related important open questions in modern astrophysical research: how do galaxies evolve over their lifetimes, possibly changing their appearance and

Main objective of this project is to maximize the scientific exploitation of the unique capabilities of SONG (Stellar Observations Network Group) high-precision radial velocity measurements and flexibility to execute robotic observations over long periods of time- on scientific programs up to now not achievable with any other space or ground based

Ramón y Cajal contract to develop his research work in the specific research project “The integrated galactic stellar initial mass function - connecting resolved and unresolved stellar populations”.