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

  • Retrieving day- and nightside atmospheric properties of the ultra-hot Jupiter TOI-2109b: Detection of Fe and CO emission lines and evidence for inefficient heat transport
    The ultra-hot Jupiter (UHJ) TOI-2109b marks the lower edge of the equilibrium temperature gap between 3500 and 4500 K, an unexplored thermal regime that separates KELT-9b, the hottest planet yet discovered, from all other currently known gas giants. To study the thermochemical structure of TOI-2109b's atmosphere, we obtained high-resolution
    Cont, D. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    1
  • Red giant evolutionary status determination: The complete Kepler catalog
    Context. Evolved cool stars have three distinct evolutionary status: shell-hydrogen burning (RGB), core-helium and shell-hydrogen burning (RC), and double-shell burning (AGB). Asteroseismology can distinguish between the RC and the other status, but distinguishing RGB and AGB has been difficult seismically and spectroscopically. The precise
    Vrard, M. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    5
  • Recovering coherent flow structures in active regions using machine learning
    Analysing high-resolution solar atmospheric observations requires robust techniques to recover plasma flow features across different scales, especially in active regions. Current methodologies often fall short in capturing subgranular-scale flows, and there is limited research on the errors introduced by velocity estimation techniques and analysing
    Lennard, Matthew G. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Quiet Sun Ellerman bombs as a possible proxy for reconnection-driven spicules
    Context. Spicules are elongated, jet-like structures that populate the solar chromosphere and are rooted in the lower solar atmosphere. In recent years, high-resolution observations and advanced numerical simulations have provided insights into their properties, structures, and dynamics. However, the formation mechanism of spicules, particularly
    Sand, Mats Ola et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    1
  • Quasar Milli-lensing and Cold Dark Matter (TNG50) Subhaloes. I. Image Splitting
    We use numerical mass density profiles from the TNG50 simulation to study the impact of gravitational milli-lensing by dark matter subhaloes on the images of lensed quasars. Specifically, we study the formation of subimages and the probability of their detection. For high-concentration density profiles, the mass determines the amplitude of the
    Mediavilla, E. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Quasar microlensing in galaxy clusters as a complementary approach to intracluster light
    In the gravitational lens SDSS J1004+4112, a background quasar is lensed by a galaxy cluster, hence the light from the quasar images travels mainly through the intracluster medium. Observations in the continuum emission and the broad line region detected variability due to microlensing in the multiple images of the quasar. In this work, we use the
    Forés-Toribio, R. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0