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

  • The CARMENES TESS followup program: uncovering the most promising rocky worlds for JWST characterization
    CARMENES is an echelle spectrograph with two arms, one in the visible and one in the infrared, mounted on the 3.5 m telescope in Calar Alto Observatory, Spain. Since 2016, the CARMENES guaranteed observing time program has conducted a radial-velocity survey of 365 M dwarfs in search for planetary companions. However, over the past three years
    Palle, Enric et al.

    Fecha de publicación:

    6
    2022
    Número de citas
    0
  • TOI-1268b: The youngest hot Saturn-mass transiting exoplanet
    We report the discovery of TOI-1268b, a transiting Saturn-mass planet from the TESS space mission. With an age of less than 1 Gyr, derived from various age indicators, TOI-1268b is the youngest Saturn-mass planet known to date; it contributes to the small sample of well-characterised young planets. It has an orbital period of P = 8.1577080 ± 0
    Šubjak, J. et al.

    Fecha de publicación:

    6
    2022
    Número de citas
    10
  • TOI-178: a window into the formation and evolution of planetary systems
    Laplacian resonant chains — where astronomical bodies are in mean motion resonance with two or more other bodies — are rare phenomena observed in systems such as the TRAPPIST-1 exoplanets and the Galilean moons of Jupiter. Laplacian chains are an important tool to study the history of planetary systems occupying this configuration, as the fragility
    Hooton, Matthew J. et al.

    Fecha de publicación:

    6
    2022
    Número de citas
    0
  • TOI-2136b: a sub-Neptune planet around a nearby M3 dwarf
    Small planets with a radius between 1-4 Earth radii are extremely common in the Milky Way but their planetary formation and evolution are not revealed completely. NASA's Kepler space telescope revealed that this population has a bimodal distribution to be consistent with the transition from rocky to non-rocky planets predicted by photoevaporation
    Kawauchi, Kiyoe et al.

    Fecha de publicación:

    6
    2022
    Número de citas
    0
  • Transit Timing Variations for AU Microscopii b & c
    We explore the transit timing variations (TTVs) of the young (22 Myr) nearby AU Mic planetary system. For AU Mic b, we introduce three Spitzer (4.5 μm) transits, five TESS transits, 11 LCO transits, one PEST transit, one Brierfield transit, and two transit timing measurements from Rossiter-McLaughlin observations; for AU Mic c, we introduce three
    Wittrock, Justin M. et al.

    Fecha de publicación:

    6
    2022
    Número de citas
    0
  • V1298 Tau - Rapid contraction of giant planets?
    Current theories predict that very young giant planets have large radii and very low densities before they slowly contract to reach their final size after several hundred million years. Open stellar clusters and young moving groups of stars offer a unique opportunity to study exoplanets at their infant stages because of the well-constrained ages
    Suárez Mascareño, Alejandro

    Fecha de publicación:

    6
    2022
    Número de citas
    0