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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  • Hα kinematics of S4G spiral galaxies - III. Inner rotation curves
    We present a detailed study of the shape of the innermost part of the rotation curves of a sample of 29 nearby spiral galaxies, based on high angular and spectral resolution kinematic Hα Fabry-Perot observations. In particular, we quantify the steepness of the rotation curve by measuring its slope dRvc(0). We explore the relationship between the
    Erroz-Ferrer, S. et al.

    Fecha de publicación:

    5
    2016
    Número de citas
    29
  • Hunting down systematics in baryon acoustic oscillations after cosmic high noon
    Future dark energy experiments will require accurate theoretical predictions for the baryon acoustic oscillations (BAOs). Here, we use large N-body simulations to study any systematic shifts and damping in BAO due to non-linear effects. The impact of cosmic variance is largely reduced by dividing the tracer power spectrum by that from a `BAO-free'
    Prada, F. et al.

    Fecha de publicación:

    5
    2016
    Número de citas
    27
  • How different are the Liège and Hamburg atlases of the solar spectrum?
    Context. The high-fidelity solar spectral atlas prepared by Delbouille et al. (Liège atlas, 1973) and the atlas by Neckel (Hamburg atlas, 1999, Sol. Phys., 184, 421) are widely recognised as the most important collection of reference spectra of the Sun at disc centre in the visible wavelength range. The two datasets serve as fundamental resources
    Doerr, H.-P. et al.

    Fecha de publicación:

    5
    2016
    Número de citas
    21
  • High ionisation absorption in low mass X-ray binaries
    The advent of the new generation of X-ray telescopes yielded a significant step forward in our understanding of ionised absorption generated in the accretion discs of X-ray binaries. It has become evident that these relatively weak and narrow absorption features, sporadically present in the X-ray spectra of some systems, are actually the signature
    Ponti, G. et al.

    Fecha de publicación:

    5
    2016
    Número de citas
    41
  • GU Monocerotis: A high-mass eclipsing overcontact binary in the young open cluster Dolidze 25
    Context. The eclipsing binary GU Mon is located in the star-forming cluster Dolidze 25, which has the lowest metallicity measured in a Milky Way young cluster. Aims: GU Mon has been identified as a short-period eclipsing binary with two early B-type components. We set out to derive its orbital and stellar parameters. Methods: We present a
    Lorenzo, J. et al.

    Fecha de publicación:

    5
    2016
    Número de citas
    12
  • Earth's albedo variations 1998-2014 as measured from ground-based earthshine observations
    The Earth's albedo is a fundamental climate parameter for understanding the radiation budget of the atmosphere. It has been traditionally measured not only from space platforms but also from the ground for 16 years from Big Bear Solar Observatory by observing the Moon. The photometric ratio of the dark (earthshine) to the bright (moonshine) sides
    Palle, E. et al.

    Fecha de publicación:

    5
    2016
    Número de citas
    13