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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  • Characterisation of the new target of the NASA Lucy mission: Asteroid 152830 Dinkinesh (1999 VD57)
    Context. The NASA Lucy mission is designed to collect data that will be used to study the very interesting population of Jupiter Trojans, which are considered to be time capsules from the time of birth of our Solar System. During its journey, the mission will pass near a main belt asteroid, Donaldjohanson. Recently, NASA announced that a new
    de León, J. et al.

    Fecha de publicación:

    4
    2023
    Número de citas
    5
  • Chemical characterisation of the X-shooter Spectral Library (XSL): [Mg/Fe] and [Ca/Fe] abundances
    Context. The X-shooter Spectral Library (XSL) is a large empirical stellar library used as a benchmark for the development of stellar population models. The inclusion of α-element abundances is crucial to disentangling the chemical evolution of any stellar system. Aims: The aim of this paper is to provide a catalogue of high-precision, accurate
    Santos-Peral, P. et al.

    Fecha de publicación:

    4
    2023
    Número de citas
    0
  • Near-ultraviolet absorption distribution of primitive asteroids from spectrophotometric surveys. I. Radial distribution
    Context. Hydrated minerals, such as phyllosilicates, on asteroids can provide constraints on the temperature or compositional distribution of the early Solar System. Previous studies pointed out the possibility that absorption in the near-ultraviolet (NUV, 0.35-0.5 μm) wavelength region is a proxy for hydrated minerals in primitive asteroids
    Tatsumi, E. et al.

    Fecha de publicación:

    4
    2023
    Número de citas
    3
  • Temporal Structures in Electron Spectra and Charge Sign Effects in Galactic Cosmic Rays
    We present the precision measurements of 11 years of daily cosmic electron fluxes in the rigidity interval from 1.00 to 41.9 GV based on 2.0 ×10 8 electrons collected with the Alpha Magnetic Spectrometer (AMS) aboard the International Space Station. The electron fluxes exhibit variations on multiple timescales. Recurrent electron flux variations
    Aguilar, M. et al.

    Fecha de publicación:

    4
    2023
    Número de citas
    7
  • Confirmation of Color-dependent Centroid Shift Measured After 1.8 Years with HST
    We measured the precise masses of the host and planet in the OGLE-2003-BLG-235 system, when the lens and source were resolving, with 2018 Keck high resolution images. This measurement is in agreement with the observation taken in 2005 with the Hubble Space Telescope (HST). In the 2005 data, the lens and sources were not resolved and the measurement
    Bhattacharya, Aparna et al.

    Fecha de publicación:

    5
    2023
    Número de citas
    2
  • A sub-Neptune transiting the young field star HD 18599 at 40 pc
    Transiting exoplanets orbiting young nearby stars are ideal laboratories for testing theories of planet formation and evolution. However, to date only a handful of stars with age <1 Gyr have been found to host transiting exoplanets. Here we present the discovery and validation of a sub-Neptune around HD 18599 , a young (300 Myr), nearby (d = 40 pc)
    de Leon, J. P. et al.

    Fecha de publicación:

    6
    2023
    Número de citas
    4