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

  • Black hole and massive galaxy evolution
    Our theoretical understanding of cosmology is, a priori, inconsistent with observations. In a Universe dominated by dark matter, the most massive galaxies are expected to form late and slowly, which is in contradiction with observations whose behavior is just the opposite. In a scenario where our theoretical conception of the Universe is in
    Ignacio
    Martín Navarro
    In force date
    Not in force
  • "Studying the physics of inflation through observations of the Cosmic Microwave Background from the Teide Observatory"
    The final goal of this project is to guarantee the scientific explotation of the data coming from the QUIJOTE and GroundBIRD experiments, both currently located at the Teide Observatory with the aim of performing highaccuracy observations of the Cosmic Microwave Background (CMB) polarisation.The final goal of these observations is the detection of
    Ricardo Tanausú
    Genova Santos
    In force date
    Not in force
  • Search, impact and fundamental properties of Ultra-compact X-ray binaries
    The vast majority of the known galactic population of stellar-mass black holes and a significant fraction of the neutron stars are found in X-ray binary systems. Among them, the population of ultra-compact X-ray binaries (UCXBs) is of particular interest, as they harbour degenerate donor stars that feed the black-hole/neutron star with hydrogen
    Montserrat
    Armas Padilla
    In force date
    Not in force
  • Stellar populations models with  varying abundance element ratios to constrain galaxy formation timescales
    The formation and evolution of galaxies is considered one of the hottest topics in Modern Astronomy. Studies on their stellar content have provided severe restrictions on their formation processes. A key result is that galaxies show abundances element ratios that differ from those found in the solar neighborhood. The abundance patterns are
    Alexandre
    Vazdekis Vazdekis
    In force date
    Not in force
  • Development of the FRIDA control software during the Integration and Testing phases
    The FRIDA instrument is an integral field spectrograph and camera, both designedto work in high spatial resolution, at the diffraction limit of GTC (Gran Telescopio Canarias), in the range of 1 - 2.5 microns. FRIDA is a general purpose instrument for the entire GTC community, its construction approved by the Scientific Advisory Committee of GTC in
    José Alfonso
    López Aguerri
    In force date
    Not in force
  • Scientific analysis of ultra-deep astronomical images
    One of the projects with the greatest impact currently being developed by the Instituto de Astrofísica de Canarias is the state-of-the-art analysis of optical astronomical images and, in particular, the study of objects with ultra-faint surface brightness. We have already made a number of scientific discoveries that have been made possible, not
    Johan Hendrik
    Knapen Koelstra
    In force date
    Not in force