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

  • 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
  • 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, later, also from the University of Las Palmas de Gran Canaria and other universities, whose objective is to develop its own space mission. In particular, the goal is to design, manufacture
    Alejandro
    Oscoz Abad
    In force date
    Not in force
  • 2D spectroscopy of planetary nebulae with high abundance discrepancies
    The discrepancy between chemical abundances calculated from optical recombination lines (RLs) and collisional excitation lines (CELs) is an important unsolved problem in nebular astrophysics. In planetary nebulae (PNe) there is increasing evidence that the discrepancy is due to the presence of two gas phases: a hot component with standard
    Jorge
    García Rojas
    In force date
    Not in force
  • Development of Big Data toos for the study of variable stars in galaxies with LSST data
    The objective of this proposal is the development of data analysis tools in preparation for the scientific exploitation of LSST, the largest mapping project of the southern sky that will begin observations in 2023. Specifically, the fundamental objective is the analysis of time series for the search and characterization of variable stars in
    Matteo
    Monelli
    In force date
    Not in force
  • Quasar feedback and molecular gas reservoirs
    The broad scientific objective of this project is to advance in our understanding of active galactic nuclei (AGN) feedback and its connection with the galaxies molecular gas reservoirs. We will do so by performing the first multiphase characterization of outflow properties in a sample of nearby and luminous type-2 quasars (QSO2s). By combining our
    Cristina
    Ramos Almeida
    In force date
    Not in force