Type of funding: Public

  • Grant
    Polarimetric inference of magnetic fields
    The magnetic field is the main driver of the spectacular activity of the solar atmosphere, which covers the photosphere, chromosphere, transition region, and...
  • Grant
    POLMAG: Polarized radiation diagnostics for exploring the magnetism of the outer solar atmosphere. ERC Advanced Grant. H2020
    POLMAG aims at a true breakthrough in the development and application of polarized radiation diagnostic methods for exploring the magnetic fields of the...
  • Grant
    PRE-EST: Preparatory Phase for the European Solar Telescope. H2020 Grant
    The objectives of the preparatory phase for EST are: (1) to explore possible legal frameworks and related governance schemes that can be used by agencies to...
  • Grant
    Precision cosmology with Planck, Quijote and SDSS
    The main goal of this project is to ensure the scientific exploitation of the experiments, missions and surveys in which the Cosmology group at the IAC is...
  • Grant
    Precision cosmology with the Cosmic Microwave Background: QUIJOTE and other microwave experiments at the Teide Observatory, and
    The main goals of this project are to cover, during the period 2020-2022, the scientific exploitation of the cosmic microwave background (CMB) experiments in...
  • Grant
    Precision cosmology with the cosmic microwave background: QUIJOTE, PLANCK and other CMB experiments at the Teide Observatory
    The main goal of this project is to ensure the scientific exploitation of the cosmic microwave background (CMB) experiments in which the IAC's cosmology group...
  • Grant
    Primitive Asteroids Spectroscopic Study: Exploitation of data from GAIA and JWST
    Asteroids are considered the residual building blocks that formed the planets: a window to the formation and evolution of our solar system. Primitive asteroids...
  • Grant
    Probing the Model Limitations of the Age Determination of Solar-like Oscillators from Space Photometry and Ground-based Spectroscopy
    The age of a star cannot be measured; it can only be inferred from comparing observational parameters with predictions from stellar models. Hereby, the...
  • Grant
    Program Stellar Variability with Rubin-LSST
    Rubin-LSST will provide an unprecedented combination of time coverage, 6-bands photometric depth and spatial extension for a variety of environments. In...