Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • The intracluster light as an estimator of the cluster mass profile
    Context. The intracluster light (ICL) comprises stars that are not bound to individual galaxies within a galaxy cluster, and it provides insights into the cluster mass distribution, evolutionary history, and dynamical state. Aims. We study the viability of the intracluster stellar mass as a proxy for computing the total mass profiles of galaxy
    Alonso Asensio, I. et al.

    Advertised on:

    8
    2025
    Citations
    0
  • The impact of rotation on the stochastic excitation of stellar acoustic modes in solar-like pulsators
    Context. Recent observational results from asteroseismic studies show that an important fraction of solar-like stars do not present detectable stochastically excited acoustic oscillations. This non-detectability seems to correlate with a high rotation rate in the convective envelope and a high surface magnetic activity. At the same time, the
    Bessila, L. et al.

    Advertised on:

    8
    2025
    Citations
    0
  • The Gondola for the SUNRISE III Balloon-Borne Solar Observatory
    SUNRISE III is a balloon-borne solar observatory dedicated to investigating the physics governing the magnetism and dynamics in the lower solar atmosphere. The observatory is designed to operate in the stratosphere, at heights around 36 km (above 99% of Earth's atmosphere), to avoid image degradation due to turbulence in the Earth's lower
    Bernasconi, Pietro et al.

    Advertised on:

    8
    2025
    Citations
    0
  • The Gaia-ESO Survey: projected rotational velocities of B stars in the Carina Nebula
    The Carina Nebula is an active star-forming region with several open clusters rich in massive OB stars, thus making it an optimal target for studying stellar properties such as rotation for large samples of these early-type stars. We studied a sample of early-type stars probable members of the eight open clusters in the Carina Complex. The
    Santos, W. et al.

    Advertised on:

    8
    2025
    Citations
    0
  • The ESPRESSO transmission spectrum of HD189733 b: Extracting the planetary sodium and lithium signatures amid stellar contamination
    Context. While transmission spectroscopy has allowed us to detect many atomic and molecular species in exoplanet atmospheres, the improvement in resolution and signal-to-noise ratio (S/N) enabled us to become sensitive to planet-occulted line distortions (POLDs) in the spectrum that are induced by center-to-limb variations (CLV) and the Rossiter
    Mounzer, D. et al.

    Advertised on:

    8
    2025
    Citations
    0
  • The entropy of galaxy spectra
    The ability of any Machine Learning method to classify the spectra of galaxies depending on the properties of the stellar component rests on the information content of the data. The well-known degeneracies found in population synthesis models suggest this information might be so entangled as to challenge the most sophisticated Deep Learning
    Ferreras, I. et al.

    Advertised on:

    8
    2025
    Citations
    0