Grant state: Granted

  • Grant
    Sunspot Oscillations: Connecting Interior and Atmospheric Layers
    Sunspots are the most evident manifestations of solar magnetism, and oscillations are a fundamental physical process taking place in them. Despite the efforts...
  • Grant
    Technological Training of IACTEC 2021
    The "Área de Carreteras, Movilidad, Innovación y Cultura" belonging to the Cabildo Insular de Tenerife, has financed the employment of IACTEC´s researchers in...
  • Grant
    Technological Training of IACTEC 2022
    The "Área de Carreteras, Movilidad, Innovación y Cultura" belonging to the Cabildo Insular de Tenerife, has financed the employment of IACTEC´s researchers in...
  • Grant
    Technological Training of IACTEC 2023
    The "Roads, Mobility, Innovation and Culture Area" belonging to the Island Council of Tenerife has financed the hiring of IACTEC researchers in the "Space"...
  • Grant
    TEIDESAT - TEchincal INvestigation and DEVelopment to SATellites
    Since its origin in December 2017, the TEIDESAT project was founded and is formed and led by a team of students, initially from the University of La Laguna and...
  • Grant
    Temporal Evolution of the Milky-way Properties from an Observational and theoretical Sinergy (GA 101066193)


    Understanding how galaxies form and evolve in the Universe is a key, long-term goal of Astrophysics. In this regard, our Galaxy provides unique insights because...
  • 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 evolution of galaxy clusters from cosmic dawn to noon
    Our overall aim is to understand the role of environment in regulating galaxy growth from the first overdensities at z~6, cosmic dawn, to the galaxy clusters...
  • 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...