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

  • Determination of the anisotropy of elementary particles with the Alpha Magnetic Spectrometer on the International Space Station
    A measurement of the cosmic ray anisotropy on the arrival directions of elementary particles (electrons, positrons and protons) has been performed in galactic coordinates by the Alpha Magnetic Spectrometer onboard the International Space Station. The analysis is based on the sample of events collected in the first 10 years of data taking. The
    Velasco, Miguel Ángel et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    0
  • Euclid preparation: L. Calibration of the halo linear bias in Λ(v)CDM cosmologies
    The Euclid mission, designed to map the geometry of the dark Universe, presents an unprecedented opportunity for advancing our understanding of the cosmos through its photometric galaxy cluster survey. Central to this endeavor is the accurate calibration of the mass- and redshift-dependent halo bias (HB), which is the focus of this paper. Our aim
    Euclid Collaboration et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    0
  • Euclid preparation: XLIX. Selecting active galactic nuclei using observed colours
    The Euclid space mission will cover over 14 000 deg 2 with two optical and near-infrared spectro-photometric instruments, and is expected to detect around ten million active galactic nuclei (AGN). This unique data set will make a considerable impact on our understanding of galaxy evolution in general, and AGN in particular. For this work we
    Euclid Collaboration et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    1
  • Exploring massive star early evolution: the case of the Herschel 36 A triple system
    Theoretical models show that some massive stars have not yet arrived at the zero-age main sequence (ZAMS) at the end of the accretion phase. At that time, they have lost their thick envelopes and thus could be optically visible. Although some candidates to optically observable ZAMS stars have been reported, the evolutionary status of none of them
    Arias, Julia I. et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    0
  • Exploring the Magnetic and Thermal Evolution of a Coronal Jet
    Coronal jets are the captivating eruptions that are often found in the solar atmosphere and primarily formed due to magnetic reconnection. Despite their short-lived nature and lower energy compared to many other eruptive events, e.g., flares and coronal mass ejections, they play an important role in heating the corona and accelerating charged
    Nayak, Sushree S. et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    0
  • Full Abundance Study of Two Newly Discovered Barium Giants
    Barium (Ba) stars are chemically peculiar stars that show enhanced surface abundances of heavy elements produced by the slow-neutron-capture process, the so-called s-process. These stars are not sufficiently evolved to undergo the s-process in their interiors, so they are considered products of binary interactions. Ba stars form when a former
    Vitali, Sara et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    0