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

  • Discovery of the local counterpart of disc galaxies at z > 4: The oldest thin disc of Milky Way using Gaia-RVS
    Context: JWST has recently detected numerous disc galaxies at high-redshifts and there have been observations of cold disc galaxies at z > 4 with ALMA. In the Milky Way, recent studies highlight the presence of metal-poor stars in cold disc orbits, suggesting an ancient disc. This prompts a fundamental question: When did the Milky Way disc form
    Nepal, Samir et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • Detector upgrade in EMIR@GTC: on-sky performances
    EMIR was shipped to the GTC on May 2016 and had its first light on June 2016. Since the beginning, the EMIR performances have been severely hampered by the many instabilities in the infrared detector, a 2048x2048 Hawaii2, built with the old original technology of the Teledyne Hawaii series. Despite of this, the instrument has proven to be powerful
    Garzón, Francisco et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • Detection of Na in the atmosphere of the hot Jupiter HAT-P-55b
    The spectral signatures of optical absorbers, when combined with those of infrared molecules, play a critical role in constraining the cloud properties of exoplanet atmospheres. We aim to use optical transmission spectroscopy to confirm the tentative color signature previously observed by multiband photometry in the atmosphere of hot Jupiter HAT-P
    Kang, Huiyi et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • Detection of Fe and Ti on the dayside of the ultrahot Jupiter MASCARA-1b with CARMENES
    Ultrahot Jupiters are a type of gaseous exoplanet that orbit extremely close to their host star, resulting in significantly high equilibrium temperatures. In recent years, high-resolution emission spectroscopy has been broadly employed in observing the atmospheres of ultrahot Jupiters. We used the CARMENES spectrograph to observe the high
    Guo, B. et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    5
  • Detection of an Earth-sized exoplanet orbiting the nearby ultracool dwarf star SPECULOOS-3
    Located at the bottom of the main sequence, ultracool dwarf stars are widespread in the solar neighbourhood. Nevertheless, their extremely low luminosity has left their planetary population largely unexplored, and only one of them, TRAPPIST-1, has so far been found to host a transiting planetary system. In this context, we present the SPECULOOS
    Gillon, Michaël et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    7
  • Deriving Star Formation Histories of Galaxies from Spectra with Simulation-based Inference
    High-resolution galaxy spectra encode information about the stellar populations within galaxies. By investigating the properties of these stars, such as their ages, masses, and metallicities, we can gain insights into the underlying physical processes that drive the growth and transformation of galaxies over cosmic time, in particular, the triggers
    Iglesias Navarro, Patricia et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0