Transparency

Economic information: Grants

Awarded

To see the Grants awarded by the IAC (Access the National Subsidy Advertising System) select "Convocatorias", Admon. del Estado: select:  Ministerio de Ciencia, Innovación e Universidades;  Organo: select: Instituto de Astrofísica de Canarias

Received

  • Weave: Cluster Surveys: A New Vision of the role of the environment in Galazy Evolution
    The environment plays a key role in the formation and evolution of galaxies. Clusters of galaxies are the most massive and virialized structures known in the Universe and therefore are the ideal laboratories for the study of environmental processes in galaxies. It is not an easy task to discern, between the properties of galaxies, which have been
    José Alfonso
    López Aguerri
    In force date
    Not in force
  • Kinematics of Local Group Dwarf Galaxies: Evolution, Orbits and Star Formation Quenching
    The Local Group (LG) offers us a chance to test the present scenario of galaxy formation in ways that are impossible elsewhere. It contains about 50 know galaxies, most of which are dwarfs so faint that they would not be detected beyond the LG. Hence, ourunderstanding of low-mass galaxy formation physics, strongly tied to models of galaxy feedback
    Antonio
    Aparicio Juan
    In force date
    Not in force
  • Galaxy Clusters: abundance, formation and evolution from a cosmological approach
    This proposal seeks the scientific exploitation of the project on Dynamics of cool-core galaxy clusters, the mapping Cosmological Galaxy Clusters, and the galaxy cluster surveys of the EUCLID space mission in the coming years. The objectives of the project here presented are: 1) To investigate the nature of galaxy clusters with cool-cores, their
    Rafael Delfin
    Barrena Delgado
    In force date
    Not in force
  • RR Lyrae stars, a lighthouse to the distant Universe and the early evolution of galaxies
    The general objective of this project is to exploit the potential of the Gaia mission, combined with the database built by our team in the last years, to bring substantial improvement in the determination of stellar distances and the early evolution of the LG galaxies. We will combine high resolution spectroscopy, optical and NIR photometric time
    Matteo
    Monelli
    In force date
    Not in force
  • 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 among the oldest in the Universe, thick discs are relics of the infancy of galaxies. Thus, understanding the origin of thick discs is key to unveil how galaxies themselves form, which in turn
    Sébastien
    Comerón Limbourg
    In force date
    Not in force
  • Scientific explotation of the new ESPRESSO, NIRPS and Horus spectrographs for the study of exoplanets and the most primitive stars of the Milky Way
    High-resolution, high-stability spectroscopy is crucial for the precise determination of radial velocities and the detailed chemical analysis of stars in different contexts of the Galaxy. The ESPRESSO and HORuS spectrographs, in operation on the VLT and GTC telescopes since mid-2018, are already contributing significantly to our knowledge of
    Jonay Isai
    González Hernández
    In force date
    Not in force