Type of funding: Public

  • Grant
    The reionization of the universe
    The Universe's re-ionisation is at the forefront of research. How the re-ionisation occurred is however still not known. This project intents to understand the...
  • Grant
    The role of starbursts in formation and evolution of galaxies: ESTALLIDOS 5.
    Starsbursts play a key role in the cosmic evolution of galaxies. There is an intimate link between the average star formation (SF) rate history of the universe...
  • Grant
    The structure and evolution of galaxies and their central regions
    We propose to study the evolution of galaxies through detailed analysis of observational data obtained with the most modern ground- and space-based telescopes...
  • Grant
    The structure and evolution of galaxies and their outskirts
    We propose to study the evolution of galaxies through detailed analysis of observational data obtained with the most modern ground- and space-based telescopes...
  • Grant
    The structure and evolution of the galaxies and their central regions
    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...
  • Grant
    The whole sun project: untangling the complex physical mechanisms behind our eruptive star and its twins: "Whole sun"
    The Sun is a magnetically active star with violent eruptions that can hit Earth´s magnetosphere and cause important perturbations in our technology-dependent...
  • Grant
    Thick discs, relics of the infancy of galaxies
    Galaxy discs are made of two components, the thin and the thick disc. Thick discs contain up to 50% of the baryonic mass of a galaxy. Because their stars are...
  • Grant
    Towards the characterization of planetary atmospheres and the search for life: Cheops, Carmenes
    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...
  • Grant
    Towards the understanding of the late stages of stellar evolution and the formation of complex organic molecules
    Most of the stars (M < 8 solar masses, Ms) end their lives with a phase of strong mass loss on the Asymptotic Giant Branch (AGB), just before they form...