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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  • Measurements of t t ¯ spin correlations and top quark polarization using dilepton final states in p p collisions at √{s }= 8 TeV
    Measurements of the top quark-antiquark (t t ¯ ) spin correlations and the top quark polarization are presented for t t ¯ pairs produced in p p collisions at √{s }=8 TeV . The data correspond to an integrated luminosity of 19.5 fb-1 collected with the CMS detector at the LHC. The measurements are performed using events with two oppositely charged
    Khachatryan, V. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    66
  • LOFAR MSSS: detection of a low-frequency radio transient in 400 h of monitoring of the North Celestial Pole
    We present the results of a four-month campaign searching for low-frequency radio transients near the North Celestial Pole with the Low-Frequency Array (LOFAR), as part of the Multifrequency Snapshot Sky Survey (MSSS). The data were recorded between 2011 December and 2012 April and comprised 2149 11-min snapshots, each covering 175 deg2. We have
    Stewart, A. J. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    68
  • Inferring planetary obliquity using rotational and orbital photometry
    The obliquity of a terrestrial planet is an important clue about its formation and critical to its climate. Previous studies using simulated photometry of Earth show that continuous observations over most of a planet's orbit can be inverted to infer obliquity. However, few studies of more general planets with arbitrary albedo markings have been
    Schwartz, J. C. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    43
  • Heating of the Partially Ionized Solar Chromosphere by Waves in Magnetic Structures
    In this paper, we show a “proof of concept” of the heating mechanism of the solar chromosphere due to wave dissipation caused by the effects of partial ionization. Numerical modeling of non-linear wave propagation in a magnetic flux tube, embedded in the solar atmosphere, is performed by solving a system of single-fluid quasi-MHD equations, which
    Shelyag, S. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    61
  • Erratum: “Results of a Search for γ Dor and δ Sct Stars with the Kepler Spacecraft” (2015, AJ, 149, 68)
    Not Available
    Jackiewicz, J. et al.

    Fecha de publicación:

    3
    2016
    Número de citas
    1