Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Homogeneity in the early chemical evolution of the Sextans dwarf spheroidal galaxy
    We present the high-resolution spectroscopic analysis of two new extremely metal-poor star (EMPS) candidates in the dwarf spheroidal galaxy Sextans. These targets were preselected from medium-resolution spectra centered around the Ca II triplet in the near-infrared and were followed-up at higher resolution with VLT/UVES. We confirm their low
    Lucchesi, R. et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    18
  • HARMONI: first light spectroscopy for the ELT: instrument final design and quantitative performance predictions
    HARMONI is the adaptive optics assisted, near-infrared and visible light integral field spectrograph for the Extremely Large Telescope (ELT). A first light instrument, it provides the work-horse spectroscopic capability for the ELT. As the project approaches its Final Design Review milestone, the design of the instrument is being finalized, and the
    Thatte, Niranjan A. et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    10
  • HARMONI science path optics: predicting and analysing the expected as-built performance with and end-to-end optical model
    HARMONI, an adaptive optics (AO) assisted integral field spectrograph (IFS), will be the core spectroscopic capability for the European Southern Observatory's (ESO's) Extremely Large Telescope (ELT). It will support several AO modes and achieve diffraction-limited (≈10 mas) to seeing-limited spatial resolution, at low to high spectral resolving
    Tecza, Matthias et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    0
  • HADES RV programme with HARPS-N at TNG. XII. The abundance signature of M dwarf stars with planets
    Context. Most of our current knowledge on planet formation is still based on the analysis of main sequence, solar-type stars. Conversely, detailed chemical studies of large samples of M dwarfs hosting planets are still missing. Aims: Correlations exist between the presence of different types of planets around FGK stars and metallicity, individual
    Maldonado, J. et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    62
  • H2020 opticon WP5 overview: investigating the use of additive manufacturing AM) for the design and build of multifunctional integrated astronomical components
    Additive manufacturing (AM) methods and post processing techniques are promising methodologies considering that it is now possible to print in a wide variety of materials using processes much refined from those originally available twenty years ago. To date the uptake of AM in Astronomy is relatively low compared to other application areas
    Schnetler, Hermine et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    0
  • GATOS: A fast multi-channel imager and spectrograph for the Gran Telescopio Canarias
    GATOS (GTC Astrophysical Transient Octuple-channel imaging Spectrograph) is a multi-channel imager and spectrograph capable of simultaneously obtaining images of the same field in 8 optical and near-infrared bands or alternatively performing spectroscopy covering the range between 3500 and 23500 Angstrom in a single shot at a resolving power of R ∼
    de Ugarte Postigo, A. et al.

    Fecha de publicación:

    12
    2020
    Número de citas
    0