Financing logos: EU FEDER

  • Grant
    Contribution of the IAC to space missions: Developments for SPICA and Athena, Herschel post-operations and multi-frequency scientific exploitation
    In the last two decades, Spain has built up strong IR and X-ray communities which have successfully contributed, at Co-I level, to the construction and to the...
  • Grant
    Contribution of the IAC to the space mission plato 2.0 phases b2 / c
    This subproject aims to contribute with for scientific and technical work for the IACs contributions to the PLATO 2.0 mission is requested. This includes...
  • Grant
    COordinating BEARD: The Challenge of Milky Way-like Galaxies to the Cold Dark Matter Paradigm
    In a Universe dominated by Cold Dark Matter (CDM), the growth of galaxies is expected to happen hierarchically: mergers of small systems eventually create a...
  • Grant
    Cosmic microwave background from the OT: QUIJOTE and other experiments
    The main goal of this project is to consolidate and to guarantee the scientific leadership of those CMB experiments operating from the Teide Observatory (OT)...
  • Grant
    Cosmic Microwave Background, QUIJOTE experiment
  • Grant
    Cosmic microwave background: Quijote experiment
    The IAC cosmology group leads the QUIJOTE experiment, which is a unique project in the polarization of the Cosmic Microwave Background, consisting of two...
  • Grant
    Cosmological tests and study of the innermost regions of quasars from observations of gravitational lenses
    Gravitational lenses are a powerful tool for Astrophysics and Cosmology. We will combine the experience of our group in theory and observation of gravitational...
  • Grant
    Cosmology at all redshifts: Exploitation and preparatory work for J-PLUS, J-PAS, QUIJOTE, and LiteBIRD
    The proposed research is organized around two different fronts of activity: (1) Preparatory and exploratory work towards the study of the Large Scale Structure...
  • Grant
    Cryogenic technologies for large instruments
    The dimensions of the instruments in design for the next generation of large telescopes exceed the capacities of the cryogenic and vacuum infrastructures...