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..

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  • A transiting M-dwarf showing beaming effect in the field of Ruprecht 147
    We report the discovery and characterization of an eclipsing M5Vdwarf star, orbiting a slightly evolved F7V main sequence star. In contrast to previous claims in the literature, we confirm that the system does not belong to the galactic open cluster Ruprecht 147. We determine its fundamental parameters combining K2 time-series data with
    Eigmüller, P. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    8
  • A Large Ground-based Observing Campaign of the Disintegrating Planet K2-22b
    We present 45 ground-based photometric observations of the K2-22 system collected between 2016 December and 2017 May, which we use to investigate the evolution of the transit of the disintegrating planet K2-22b. Last observed in early 2015, in these new observations we recover the transit at multiple epochs and measure a typical depth of
    Colón, Knicole D. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    10
  • A Framework for Prioritizing the TESS Planetary Candidates Most Amenable to Atmospheric Characterization
    A key legacy of the recently launched the Transiting Exoplanet Survey Satellite (TESS) mission will be to provide the astronomical community with many of the best transiting exoplanet targets for atmospheric characterization. However, time is of the essence to take full advantage of this opportunity. The James Webb Space Telescope (JWST), although
    Kempton, E. M.-R. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    487
  • A chemical survey of exoplanets with ARIEL
    Thousands of exoplanets have now been discovered with a huge range of masses, sizes and orbits: from rocky Earth-like planets to large gas giants grazing the surface of their host star. However, the essential nature of these exoplanets remains largely mysterious: there is no known, discernible pattern linking the presence, size, or orbital
    Tinetti, Giovanna et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    349
  • A candidate super-Earth planet orbiting near the snow line of Barnard's star
    Barnard's star is a red dwarf, and has the largest proper motion (apparent motion across the sky) of all known stars. At a distance of 1.8 parsecs1, it is the closest single star to the Sun; only the three stars in the α Centauri system are closer. Barnard's star is also among the least magnetically active red dwarfs known2,3 and has an estimated
    Ribas, I. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    135
  • When binaries keep track of recent nucleosynthesis. The Zr-Nb pair in extrinsic stars as an s-process diagnostic
    Context. Barium stars are s-process enriched giants. They owe their chemical peculiarities to a past mass transfer phase. During this phase they were polluted by their binary companion, which at the time was an asymptotic giant branch (AGB) star, but is now an extinct white dwarf. Barium stars are thus ideal targets for understanding and
    Karinkuzhi, D. et al.

    Fecha de publicación:

    10
    2018
    Número de citas
    44