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 Resolved Magnetically Split Lines in SDSS/APOGEE Spectra of 157 Ap/Bp Stars
    We report on magnetic field measurements of 157 chemically peculiar A/B stars (Ap/Bp) based on resolved, magnetically split absorption lines present in H-band spectra provided by the Sloan Digital Sky Survey (SDSS)/Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey. These stars represent the extreme magnetic end of a still
    Chojnowski, S. Drew et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    32
  • Discovery of a lensed ultrabright submillimeter galaxy at z=2.0439
    We report an ultra-bright lensed submillimeter galaxy (SMG) at z=2.0439, WISE J132934.18+224327.3, identified as a result of a full-sky cross-correlation of the AllWISE and Planck compact source catalogs aimed to search for bright analogs of the submillimeter galaxy SMMJ2135, the Cosmic Eyelash. Inspection of archival SCUBA-2 observations of the
    Díaz-Sánchez, A. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    0
  • Diagnostic potential of the Ca II 8542 Å line for solar filaments
    Aims: In this study we explore the diagnostic potential of the chromospheric Ca II line at 8542 Å for studying the magnetic and dynamic properties of solar filaments. We have acquired high spatial resolution spectropolarimetric observations in the Ca II 8542 Å line using the CRISP instrument at the Swedish 1 m Solar Telescope. Methods: We used the
    Díaz Baso, C. J. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    21
  • Detection and Doppler monitoring of K2-285 (EPIC 246471491), a system of four transiting planets smaller than Neptune
    Context. The Kepler extended mission, also known as K2, has provided the community with a wealth of planetary candidates that orbit stars typically much brighter than the targets of the original mission. These planet candidates are suitable for further spectroscopic follow-up and precise mass determinations, leading ultimately to the construction
    Palle, E. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    22
  • Detection and characterization of an ultra-dense sub-Neptunian planet orbiting the Sun-like star K2-292
    We present the discovery and characterization of a new transiting planet from Campaign 17 of the Kepler extended mission K2. The planet K2-292 b is a warm sub-Neptune on a 17 day orbit around a bright (V = 9.9 mag) solar-like G3 V star with a mass and radius of M⋆ = 1.00 ± 0.03 M⊙ and R⋆ = 1.09 ± 0.03 R⊙, respectively. We modeled simultaneously the
    Luque, R. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    24
  • Deep Learning for morphological classification of galaxies
    Galaxies exhibit a wide variety of morphologies which are strongly related to their star formation histories. Having large samples of morphologically classified galaxies is fundamental to understand their formation and evolution. Morphological classification of galaxies based on visual inspection is extremely time consuming: an impossible task when
    Domínguez Sánchez, H. et al.

    Fecha de publicación:

    3
    2019
    Número de citas
    0