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

  • Cross-correlation transmission spectroscopy of ultra-hot Jupiters WASP-189b, HAT-P-57b, KELT-17b, and KELT-21b with GIANO-B
    Since the discovery of the first exoplanet, significant efforts have been made to characterise their atmospheres. Ultra-hot Jupiters (UHJs) are of particular interest due to their extended and hot atmospheres. Although previous studies have focused on the detection of atomic species at optical wavelengths, near-infrared (NIR) observations offer the
    Meni-Gallardo, P. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • Chromospheric Dynamics of an Umbral Flare Kernel-Based on Coordinated SUNRISE III SCIP and Domeless Solar Telescope Observations
    We report imaging spectroscopic observations of an M1.4 solar flare obtained during a coordinated observation between the infrared spectropolarimeter SCIP onboard the SUNRISE III balloon mission and Domeless Solar Telescope (DST) at Hida Observatory, Kyoto University. The flare that occurred on 2024 July 13 in NOAA Active Region 13738 exhibited a
    Asai, Ayumi et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • CHEOPS photometry from 2024 reveals a reversal in the transit-timing variations of AU Mic c
    We present new CHEOPS transit observations of AU Mic b and AU Mic c obtained between June and September 2024, extending the baseline of transit-timing measurements of this young planetary system. For AU Mic b, the timing signal is well established, with a semi-amplitude (10 ± 3 min) and a characteristic modulation timescale (1168 ± 20 d) consistent
    Garai, Z. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • Characterizing Candidate Blazar Counterparts of the Ultra-high-energy Event KM3-230213A
    High-energy astrophysical neutrinos serve as crucial messengers for understanding hadronic acceleration processes and identifying the origins of cosmic rays, with blazars among the most promising neutrino sources. The KM3NeT experiment reported the detection of an ultrahigh-energy neutrino with an energy estimate of ~220 PeV, the most energetic yet
    Adriani, O. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    67
  • Challenging the archetypal intermittent radio galaxy J0111+3906: New insights from optical GTC/OSIRIS and radio VLA and LOFAR observations
    We present results on new optical Gran Telescopio CANARIAS OSIRIS+ spectroscopy and radio Very Large Array (VLA) observations at 360 MHz of the optical object behind the radio emission 20 arcseconds east of the archetypal restarted compact symmetric object (CSO) J0111+3906. The optical counterpart is a post-starburst galaxy at redshift z = 1.042
    Orienti, M. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • Cause of Chromospheric Opposite Polarity Intrusions Discovered in Sunrise III/SCIP Data: MURaM-ChE Simulations Point to Twisted Flux Ropes
    The Sunrise Chromospheric Infrared spectroPolarimeter (SCIP) instrument on board the balloon-borne SUNRISE III observatory provided new high-resolution observations of the solar chromosphere in the Ca II λ854.2 nm line. The Stokes V signal in magnetic network regions was found to show fine-structured details, which suggests the magnetic field above
    Ondratschek, Patrick A. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    1