Financing logos: Ministerio de Ciencia, Innovación y Universidades

  • Grant
    The Baryonic Cycle and its Stellar populations
    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...
  • Grant
    The central PARSEC of galaxies, Adaptive Optics instrumentation development
    PARSEC is a multiwavelength investigation of the centre of the nearest galaxies at parsecs scale. It studies the brightest mv <19 mag, and nearest up to ~ 20...
  • Grant
    The Local Group in Multi-Dimensions: Probing Galaxy Evolution with Structures, Chemo-dynamics and Star Formation Histories of resolved galaxies
    We propose to investigate fundamental questions concerning the formation and evolution of galaxies, from the smallest galactic scales to those of large spiral...
  • Grant
    The Multiple Early Channels of EvolutioN of mAssive Stars
    Massive stars are those with more than ~8 solar masses, the limit above which stars may undergo a core collapse supernova (SN) explosion at the end of its life...
  • News
    The number of visitors to GRANTECAN is greater than 10,000 per year and a new surround exhibit is opened
    The Gran Telescopio Canarias or GRANTECAN has surpassed, for the first time, the 10,000 face-to-face visits. The forecast is that by the end of the year there...
  • Grant
    The physics of the Solar Atmosphere: theory, radiation diagnostics and supercomputing
    The Sun, our star, is not only the source of the electromagnetic radiation that bathes our planet; it also sweeps the Earth's magnetosphere with its wind and...
  • 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
    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
    Tracking active galactic nuclei feedback from parsec to kiloparsec scales
    Active galactic nuclei (AGN) feedback is the effect that nuclear activity produces in the interstellar and circumgalactic medium (ISM and CGM) of galaxies...