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

  • MOA-2007-BLG-400 A Super-Jupiter-mass Planet Orbiting a Galactic Bulge K-dwarf Revealed by Keck Adaptive Optics Imaging
    We present Keck/NIRC2 adaptive optics imaging of planetary microlensing event MOA-2007-BLG-400 that resolves the lens star system from the source. We find that the MOA-2007-BLG-400L planetary system consists of a 1.71 ± 0.27M Jup planet orbiting a 0.69 ± 0.04M ⊙ K-dwarf host star at a distance of 6.89 ± 0.77 kpc from the Sun. So, this planetary
    Bhattacharya, Aparna et al.

    Fecha de publicación:

    8
    2021
    Número de citas
    25
  • Dust environment of active asteroids P/2019 A4 (PANSTARRS) and P/2021 A5 (PANSTARRS)
    We report on the characterization of the dust activity and dynamical evolution of two faint active asteroids, P/2019 A4, and P/2021 A5, observed with the 10.4 m GTC using both imaging and spectroscopy. Asteroid P/2019 A4 activity is found to be linked to an impulsive event occurring some ±10 d around perihelion, probably due to a collision or a
    Moreno, Fernando et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    10
  • Local variations of the Stellar Velocity Ellipsoid-I: the disc of galaxies in the Auriga simulations
    The connection between the Stellar Velocity Ellipsoid (SVE) and the dynamical evolution of galaxies has been a matter of debate in the last years and there is no clear consensus whether different heating agents (e.g. spiral arms, giant molecular clouds, bars and mergers) leave clear detectable signatures in the present day kinematics. Most of these
    Walo-Martín, Daniel et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    4
  • Pushing automated morphological classifications to their limits with the Dark Energy Survey
    We present morphological classifications of ~27 million galaxies from the Dark Energy Survey (DES) Data Release 1 (DR1) using a supervised deep learning algorithm. The classification scheme separates: (a) early-type galaxies (ETGs) from late-type galaxies (LTGs); and (b) face-on galaxies from edge-on. Our convolutional neural networks (CNNs) are
    Vega-Ferrero, J. et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    41
  • The lens SW05 J143454.4+522850: a fossil group at redshift 0.6?
    Fossil groups are considered the end product of natural galaxy group evolution in which group members sink towards the centre of the gravitational potential due to dynamical friction, merging into a single, massive, and X-ray bright elliptical. Since gravitational lensing depends on the mass of a foreground object, its mass concentration, and
    Denzel, Philipp et al.

    Fecha de publicación:

    9
    2021
    Número de citas
    0
  • Spectral diversity of the inner belt primitive asteroid background population
    We present new near-infrared spectra of 55 objects observed using the NASA InfraRed Telescope Facility and the Telescopio Nazionale Galileo, along with visible spectra of 21 objects obtained from the SMASS and S 3OS 2 surveys, to explore the differences in spectral slope and curvature between the background and the families and to show that the
    Arredondo, Anicia et al.

    Fecha de publicación:

    11
    2021
    Número de citas
    1