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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  • NEOMIR: a space based infrared mission for NEO detection, characterization and early warning
    Most current and planned near-Earth objects (NEO) surveys are made with ground-based telescopes and carried out in the visible wavelength range. However, this approach has some limitations, such as (1) weather dependency, (2) only a portion of the night sky is visible from any given location on Earth, (3) NEOs are difficult to detect at low
    Licandro, Javier et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0
  • MUSE spectroscopy of the high abundance discrepancy planetary nebula NGC 6153
    Context. The abundance discrepancy problem in planetary nebulae (PNe) has long puzzled astronomers. NGC 6153, with its high abundance discrepancy factor (ADF ~ 10), provides a unique opportunity to study the chemical structure and ionisation processes within these objects. Aims. We aim to understand the chemical structure and ionisation processes
    Gómez-Llanos, V. et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    4
  • Measuring stellar surface rotation and activity with the PLATO mission: I. Strategy and application to simulated light curves
    The Planetary Transits and Oscillations of stars mission (PLATO) will allow us to measure surface rotation and monitor photometric activity of tens of thousands of main sequence solar-type and subgiant stars. This paper is the first of a series dedicated to the preparation of the analysis of stellar surface rotation and photospheric activity with
    Breton, S. N. et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    7
  • Massive characterisation of subgiants and red giants with TESS (Kepler and Gaia)
    TESS serves as a formidable tool for investigating stellar variability. Nonetheless, the adaptation of methodologies employed in other space missions, such as Kepler, to deduce long stellar rotation periods or solar-like stellar pulsations has been a challenge. The advent of multiple sectors of data for most stars every two years with the extended
    García, Rafael A. et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0
  • Magnetic field diagnostics of prominences with the Mg II k line 3D Stokes inversions versus traditional methods
    The Mg II k resonance line is commonly used for diagnosing the solar chromosphere. We theoretically investigated its intensity and polarization in solar prominences, taking 3D radiative transfer and Hanle and Zeeman effects into account. We used an optically thick 3D model representative of a solar prominence and applied several inversion methods
    Štěpán, Jiří et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    2
  • Machine Learning for Future Hyperspectral Data Analysis with the Hyperscout-H instrument on the ESA's Hera Mission
    Introduction Hera is ESA's first planetary defense mission designed to characterize the binary near-Earth asteroid (65803) Didymos [1]. Its secondary component, Dimorphos, was the target of the large-scale controlled collision with the NASA/DART spacecraft in September 2022 [2]. Thus, the Hera mission will provide an unprecedented opportunity to
    Pantelimon Prodan, George et al.

    Fecha de publicación:

    9
    2024
    Número de citas
    0