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

  • The Cosmological Optical Convergence: Extragalactic Background Light from TeV Gamma Rays
    The intensity of the extragalactic background (EBL), the accumulated optical and infrared emissions since the first stars, is the subject of a decades-long tension in the optical band. These photons form a target field that attenuates the γ-ray flux from extragalactic sources. This Letter reports the first γ-ray measurement of the EBL spectrum at z
    Gréaux, Lucas et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    3
  • SWEET-Cat: A view on the planetary mass-radius relation
    Aims. SWEET-Cat (Stars With ExoplanETs Catalog) was originally introduced in 2013, and since then, the number of confirmed exoplanets has increased significantly. A crucial step for a comprehensive understanding of these new worlds is the precise and homogeneous characterization of their host stars. Methods. We used a large number of high
    Sousa, S. G. et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    1
  • Study of the excitation of large-amplitude oscillations in a prominence by nearby flares
    Context. Large-amplitude oscillations are a common occurrence in solar prominences. These oscillations are triggered by energetic phenomena such as jets and flares. On March 14–15, 2015, a filament partially erupted in two stages, leading to oscillations in different parts of it. Aims. In this study, we aim to explore the longitudinal oscillations
    Luna, Manuel et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    2
  • Standardised formats and open-source analysis tools for the MAGIC telescopes data
    Instruments for gamma-ray astronomy at Very High Energies ( E > 100 GeV) have traditionally derived their scientific results through proprietary data and software. Data standardisation has become a prominent issue in this field both as a requirement for the dissemination of data from the next generation of gamma-ray observatories and as an
    Kluge, G. W. et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    0
  • Seismic differences between solar magnetic cycles 23 and 24 for low-degree modes
    Solar magnetic activity follows regular cycles of about 11 years with an inversion of polarity in the poles every ∼22 years. This changing surface magnetism impacts the properties of the acoustic modes. The acoustic mode frequency shifts are a good proxy of the magnetic cycle. In this Letter we investigate solar magnetic activity cycles 23 and 24
    García, R. A. et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    1
  • Recovering chemical bimodalities in observed edge-on stellar disks: Insights from AURIGA simulations
    The well-known bimodal distribution of Milky Way disk stars in the [α/Fe]–metallicity plane is often used to define thick and thin disks. In external edge-on galaxies, there have been attempts to identify this type of bimodality using integral field spectroscopy (IFS) data. However, for unresolved stellar populations, observations only contain
    Pinna, Francesca et al.

    Fecha de publicación:

    11
    2024
    Número de citas
    1