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/

  • TOI-283 b: A transiting mini-Neptune in a 17.6-day orbit discovered with TESS and ESPRESSO
    Context. Super-Earths and mini-Neptunes are missing from our Solar System, yet they appear to be the most abundant planetary types in our Galaxy. A detailed characterization of key planets within this population is important for understanding the formation mechanisms of rocky and gas giant planets and the diversity of planetary interior structures
    Murgas, F. et al.

    Advertised on:

    11
    2025
    Citations
    0
  • The spatially resolved effect of mergers on the stellar mass assembly of MaNGA galaxies
    Context. Understanding the origin of stars within a galaxy, namely whether they formed in situ or were accreted from other galaxies (ex situ), is key to constraining its evolution. When they are spatially resolved, these components provide crucial insights into the mass assembly history of a galaxy. Aims. We predict the spatial distribution of the
    Angeloudi, Eirini et al.

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    11
    2025
    Citations
    0
  • The Polar Orbit of TOI-2374 b, a Planet in the Neptunian Ridge
    The "Neptunian ridge" is a recently identified peak in the frequency of planets with sizes between that of Neptune and Saturn orbiting their host stars with periods between 3 and 6 days. These planets may have formed similarly to their larger, hot Jupiter counterparts in the "3 day pileup," through a dynamically excited migration pathway. The
    Yee, Samuel W. et al.

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    11
    2025
    Citations
    0
  • The origin of the intracluster light in The Three Hundred simulations
    We investigated the origin and formation mechanisms of the intracluster light (ICL) in THE THREE HUNDRED simulations, a set of 324 hydrodynamically resimulated massive galaxy clusters. The ICL, a diffuse component comprised of stars not bound to any individual galaxy, serves as a critical tracer of cluster formation and evolution. Using two
    Contreras-Santos, A. et al.

    Advertised on:

    11
    2025
    Citations
    0
  • The IACOB project: XV. Updated calibrations of fundamental parameters of Galactic O-type stars
    Context. O-type stars are key drivers of galactic evolution. For the first time, modern spectroscopic surveys combined with Gaia distances are enabling reliable estimates of the fundamental parameters of several hundred Galactic O-type stars, spanning the full range of spectral types and luminosity classes. Aims. We aim to provide updated
    Holgado, G. et al.

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    11
    2025
    Citations
    0
  • The GECKOS survey: Jeans anisotropic models of edge-on discs uncover the impact of dust and kinematic structures
    The central regions of disc galaxies host a rich variety of stellar structures: nuclear discs, bars, bulges, and boxy-peanut bulges. These components are often difficult to disentangle, both photometrically and kinematically, particularly in star-forming galaxies where dust obscuration and complex stellar motions complicate interpretation. In this
    Rutherford, T. H. et al.

    Advertised on:

    11
    2025
    Citations
    0