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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  • Sardinia Radio Telescope observations of the Coma cluster
    We present deep total intensity and polarization observations of the Coma cluster at 1.4 and 6.6 GHz performed with the Sardinia Radio Telescope. By combining the single-dish 1.4 GHz data with archival Very Large Array observations, we obtain new images of the central radio halo and of the peripheral radio relic where we properly recover the
    Murgia, M. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    7
  • Revealing the characteristics of the dark GRB 150309A: Dust extinguished or high-z?
    Context. Dark gamma-ray bursts (GRBs) constitute a significant fraction of the GRB population. In this paper, we present a multi-wavelength analysis (both prompt emission and afterglow) of an intense (3.98 × 10 −5 erg cm −2 using Fermi-Gamma-Ray Burst Monitor) two-episodic GRB 150309A observed early on until ∼114 days post burst. Despite the strong
    Castro-Tirado, A. J. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    5
  • Probing the small-scale structure of the intergalactic medium with ESPRESSO: spectroscopy of the lensed QSO UM673
    The gravitationally lensed quasar J014516.6-094517 at z = 2.719 has been observed with the ESPRESSO instrument at the ESO VLT to obtain high-fidelity spectra of the two images A and B with a resolving power R = 70 000. At the redshifts under investigation (2.1 ≲ z ≲ 2.7), the Lyman forests along the two sightlines are separated by sub-kiloparsec
    Cristiani, Stefano et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    3
  • Predicted asteroseismic detection yield for solar-like oscillating stars with PLATO
    Aims: In this work, we determine the expected yield of detections of solar-like oscillations for the targets of the foreseen PLATO ESA mission. Our estimates are based on a study of the detection probability, which takes into account the properties of the target stars, using the information available in the PIC 1.1.0, including the current best
    Goupil, M. J. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    13
  • Orbit of the Patroclus–Menoetius Binary System and Predictions for the 2024/2025 Mutual Events Season
    We report on the ephemeris development for Menoetius, the satellite of Patroclus. Our data set consisted of ground–based and Hubble Space Telescope relative astrometry, as well as 42 lightcurves from the mutual events seasons in 2007, 2012, and 2017/2018. Our dynamical model included the effects of oblate, nonspherical shapes of the components, and
    Brozović, Marina et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • Optimizing Space Telescopes' Thermal Performance through Uncertainty Analysis: Identification of Critical Parameters and Shaping Test Strategy Development
    The integration of uncertainty analysis methodologies allows for improving design efficiency, particularly in the context of instruments that demand precise pointing accuracy, such as space telescopes. Focusing on the VINIS Earth observation telescope developed by the Instituto de Astrofísica de Canarias (IAC), this paper reports an uncertainty
    Garcia-Luis, Uxia et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    2