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

  • WEAVE: Exploring new scientific horizons through spectroscopic surveys.
    The William Herschel Telescope (WHT) has been a key player in the take-off of Spanish astronomy in the last 25 years. With the access of the Spanish community to 8-10 m (VLT, GTC) telescopes, the WHT's role is specializing in offering what major telescopes can not: large field-of-view instrumentation. In response to calls from ASTRONET and other
    José Alfonso
    López Aguerri
    In force date
    Not in force
  • WEAVE: the next-generation wide-field spectrograph for the William Herschel Telescope
    The world-class 4.2m William Herschel telescope (WHT), with its comprehensive instrument suite at the superb site of the Observatorio del Roque de los Muchachos (ORM), stood as the reference optical observational facility behind the dramatic rise in Spanish astronomy over the last 25 years. Now that the Spanish community has access to 8-10-m-class
    José Alfonso
    López Aguerri
    In force date
    Not in force
  • X-ray binaries: accretion, ejection and dynamical masses
    Black-holes and neutron stars are extremely important astrophysical objects, which become unique laboratories of extreme physics when found within X-ray binaries. Their study provides high-impact results, which are relevant for many astrophysics and fundamental physics areas. Our project target fundamental properties of both the accretion process
    Teodoro
    Muñoz Darias
    In force date
    Not in force
  • X-ray binaries: accretion, ejection and dynamical masses
    Black-holes and neutron stars are extremely important astrophysical objects, which become unique laboratories of extreme physics when found within X-ray binaries. Their study provides high-impact results, which are relevant for many astrophysics and fundamental physics areas. Our project target fundamental properties of both the accretion process
    Teodoro
    Muñoz Darias
    In force date
    Not in force
  • X-ray binaries: accretion, ejection and masses
    Accreting black-holes and neutron stars in X-ray binaries provide an ideal laboratory for exploring the physics of compact objects, yielding not only confirmation of the existence of stellar-mass black holes via dynamical mass measurements, but also the best opportunity for probing high-gravity environments and the physics of accretion; the most
    Teodoro
    Muñoz Darias
    In force date
    In force
  •  BRIDGES  - Ultracool dwarfs modeling: the bridge between planets and stars
    BRIDGES main aim is the study of physical properties of the atmospheres ultracool dwarfs andexoplanets, modelling their spectra and comparison them with observations to get their physicalparameters and study possible biomarkers of rocky planets in the habitable zones. The specific objectives planned in the context of BRIDGES are the following: SO1)
    Rafael
    Rebolo López
    In force date
    In force