Financing subprogram: SUBPROGRAMA ESTATAL DE GENERACIÓN DE CONOCIMIENTO

  • Grant
    Scientific exploitation of the NIR spectrographs EMIR and MIRADAS at the GTC
    This project is proposed with two generic objectives. On the one hand, carry out the initial scientific exploitation of the EMIR and MIRADAS instruments through...
  • Grant
    Seismology of bright stars (SONG and TESS)
    Main objective of this project is to maximize the scientific exploitation of the unique capabilities of SONG (Stellar Observations Network Group) high-precision...
  • Grant
    Solar atmosphere: theory, computational tools and support for observations
    This project aims to understand the key physical laws and processes underlying a range of basic phenomena observed in the solar atmosphere. We will study the...
  • Grant
    Solar magnetometry in the era of big telescopes
    Solar activity is produced by a variety of complex interactions between its ionized plasma and the powerful magnetic field that it creates. Studying it is...
  • Grant
    Spanish participation in the development of the HARMONI instrument for the European Extremely Large Telescope (E-ELT): "Phases of preliminary and final design"
    The ESO E-ELT (European Extremely Large Telescope) project consists primarily in building a segmented and adaptive telescope with a 40-metre-class primary...
  • Grant
    Spectropolarimetry: a window on stellar magnetism
    Magnetic fields are primary drivers of stellar formation and have profound implications on stellar evolution (on the transport of chemical species and angular...
  • Grant
    Star Formation in the Primeval Universe: Constraints from the Local Building Blocks
  • Grant
    Starbursts and evolution of galaxies
    Starsbursts play a key role in the cosmic evolution of galaxies, and so, in the star formation (SF) history of the universe, the production of metals, and the...
  • Grant
    Studies of the central galaxy parsec with high-resolution spatial techniques
    This is a multiwavelength study of the centre of the nearest and brightest galaxies at angular scales of a few parsecs. These resolutions, namely <0.1 in...