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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

  • RADIOFOREGROUNDS: Ultimate modelling of Radio foregrounds: a key ingredient for cosmology
    The aim of this project is to combine two unique datasets, the nine Planck all-sky (30-857 GHz) maps and the four QUIJOTE Northern sky (10-20 GHz) maps, to provide the best possible characterization of the physical properties of polarized emissions in the microwave domain, together with an unprecedentedly thorough description of the intensity
    José Alberto
    Rubiño Martín
    In force date
    Not in force
  • Continuous characterization of the observatories of the Canary islands
    Casiana
    Muñoz Tuñón
    In force date
    Not in force
  • Cosmic microwave background: Quijote experiment
    The IAC cosmology group leads the QUIJOTE experiment, which is a unique project in the polarization of the Cosmic Microwave Background, consisting of two telescopes and three instruments. The aim of the present action is the improvement and acquisition of equipment associated with the MFI (Multi-Frequency Instrument) instrument and the microwave
    José Alberto
    Rubiño Martín
    In force date
    Not in force
  • Towards the understanding of the late stages of stellar evolution and the formation of complex organic molecules
    Most of the stars (M < 8 solar masses, Ms) end their lives with a phase of strong mass loss on the Asymptotic Giant Branch (AGB), just before they form planetary nebulae (PNe). The strong mass loss efficiently enriches the interstellar medium (ISM) with gas and dust; AGB stars are one of the main contributors to the enrichment of the ISM where new
    Domingo Aníbal
    García Hernández
    In force date
    Not in force
  • 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 important both for purely scientific as well as practical reasons. The Sun is the only star whose surface we can resolve in detail, we can even measure its magnetic field in a more or less
    Héctor David
    Socas Navarro
    In force date
    Not in force
  • 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 momentum), as well as on the formation of planetary systems around the hosting star. Yet, stellar magnetic fields are often overlooked since they are elusive, difficult to detect, and
    María Jesús
    Martínez González
    In force date
    Not in force