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 DES view of the Eridanus supervoid and the CMB cold spot
    The Cold Spot is a puzzling large-scale feature in the Cosmic Microwave Background temperature maps and its origin has been subject to active debate. As an important foreground structure at low redshift, the Eridanus supervoid was recently detected, but it was subsequently determined that, assuming the standard ΛCDM model, only about 10-20 per cent
    Kovács, A. et al.

    Fecha de publicación:

    2
    2022
    Número de citas
    26
  • The Complex Infrared Dust Continuum Emission of NGC 1068: Ground-based N- and Q-band Spectroscopy and New Radiative Transfer Models
    Thanks to ground-based infrared and submillimeter observations the study of the dusty torus of nearby active galactic nuclei has greatly advanced in the last years. With the aim of further investigating the nuclear mid-infrared emission of the archetypal Seyfert 2 galaxy NGC 1068, here we present a fitting to the N- and Q-band Michelle/Gemini
    Victoria-Ceballos, César Ivan et al.

    Fecha de publicación:

    2
    2022
    Número de citas
    6
  • Systematic KMTNet Planetary Anomaly Search. II. Six New q &lt; 2 × 10<SUP>-4</SUP> Mass-ratio Planets
    We apply the automated AnomalyFinder algorithm of Paper I to 2018-2019 light curves from the ≃13 deg 2 covered by the six KMTNet prime fields, with cadences Γ ≥ 2 hr -1. We find a total of 11 planets with mass ratios q < 2 × 10 -4, including 6 newly discovered planets, 1 planet that was reported in Paper I, and recovery of 4 previously discovered
    Mao, Shude et al.

    Fecha de publicación:

    2
    2022
    Número de citas
    46
  • System parameters of three short-period cataclysmic variable stars
    Using photometric ULTRACAM observations of three new short-period cataclysmic variables (CVs), we model the primary eclipse light curves to extract the orbital separation, masses, and radii of their component stars. We find donor masses of $0.060\pm 0.008\, {\rm M_\odot }$, $0.042\pm 0.001\, {\rm M_\odot }$, and $0.042\pm 0.004\, {\rm M_\odot }$
    Wild, J. F. et al.

    Fecha de publicación:

    2
    2022
    Número de citas
    8
  • Synthetic galaxy clusters and observations based on Dark Energy Survey Year 3 Data
    We develop a novel data-driven method for generating synthetic optical observations of galaxy clusters. In cluster weak lensing, the interplay between analysis choices and systematic effects related to source galaxy selection, shape measurement, and photometric redshift estimation can be best characterized in end-to-end tests going from mock
    Varga, T. N. et al.

    Fecha de publicación:

    2
    2022
    Número de citas
    6
  • Stellar mergers as the origin of the blue main-sequence band in young star clusters
    Recent high-quality Hubble Space Telescope photometry shows that the main-sequence stars of young star clusters form two discrete components in the colour-magnitude diagram. On the basis of their distribution in the colour-magnitude diagram, we show that stars of the blue main-sequence component can be understood as slow rotators originating from
    Wang, Chen et al.

    Fecha de publicación:

    2
    2022
    Número de citas
    57