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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  • The CARMENES search for exoplanets around M dwarfs. Planet occurrence rates from a subsample of 71 stars
    Context. The CARMENES exoplanet survey of M dwarfs has obtained more than 18 000 spectra of 329 nearby M dwarfs over the past five years as part of its guaranteed time observations (GTO) program. Aims: We determine planet occurrence rates with the 71 stars from the GTO program for which we have more than 50 observations. Methods: We use injection
    Sabotta, S. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    134
  • The atmosphere of WASP-76b seen with CARMENES: looking for CaII IRT and HeI
    Currently, one of the most used techniques to study the atmosphere of the exoplanets is transmission spectroscopy by means of high-resolution facilities (R > 105). This methodology has led to the detection of several species in the atmosphere of exoplanets, showing that ultra-hot Jupiters (Teq > 2000 K) are one of the most intriguing exoplanets
    Casasayas-Barris, Núria et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    0
  • The 4 m New Robotic Telescope Project: An Updated Report
    The New Robotic Telescope (NRT) is an international collaboration to build and operate a 4m diameter fully robotic telescope. The telescope will take advantage of the superb atmospheric conditions at the Observatory of the Roque de los Muchachos (ORM). In conjunction with a large aperture, entirely robotic operation, quick response, and a set of
    Gutiérrez, C. M. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    1
  • Symbiotic Stars in the Apache Point Observatory Galactic Evolution Experiment Survey: The Case of LIN 358 and SMC N73 (LIN 445a)
    LIN 358 and SMC N73 are two symbiotic binaries in the halo of the Small Magellanic Cloud, each composed of a hot white dwarf accreting from a cool giant companion. In this work, we characterize these systems using a combination of spectral energy distribution (SED)-fitting to the extant photometric data spanning a broad wavelength range (X-ray
    Washington, Jasmin E. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    4
  • Spectroscopic study of Ceres' collisional family candidate members: taxonomic classification and comparison to Ceres' surface.
    Despite the observed signs of large impacts on the surface of Ceres, there is no confirmed collisional family associated with this dwarf planet. Carruba et al. (2016) carried out a dynamical study in the `pristine region' of the main asteroid belt and proposed a sample of 156 asteroids as candidates to be members of a Ceres' collisional family. Our
    Tinaut-Ruano, Fernando et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    0
  • Spectrophotometric characterization of interstellar comet 2I/Borisov before perihelion passage
    Comets are primitive objects which formed in the outer parts of the proto-planetary disk, beyond the snow line. They can provide key information about the origins of our Solar System and its primordial nebula. The latest interstellar visitor [1], comet 2I/Borisov (initially designated C/2019 Q4), has given us the chance to have a probe from this
    Prodan, George P. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    0