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 local group symbiotic star population and its tenuous link with type Ia supernovae
    Context. Binary stars are gravitationally bound stellar systems where the evolution of each component can significantly influence the evolution of its companion and the system as a whole. In certain cases, the evolution of these systems can lead to the formation of a red giant-white dwarf system, which may exhibit symbiotic characteristics. Aims
    Laversveiler, Marco et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Full-Shape analysis of the power spectrum and bispectrum of DESI DR1 LRG and QSO samples
    We present the first joint analysis of the power spectrum and bispectrum using the Data Release 1 (DR1) of the Dark Energy Spectroscopic Instrument (DESI), focusing on Luminous Red Galaxies (LRGs) and quasars (QSOs) across a redshift range of 0.4 ≤ z ≤ 2.1. By combining the two- and three-point statistics, we are able to partially break the
    Novell-Masot, S. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Calibrating HMI Magnetograms Using an End-to-end Magnetograph Model
    Numerous solar and space science and operations projects rely heavily on accurate, consistent magnetic field measurements from the solar surface. These projects are hindered by well-known but poorly understood discrepancies between magnetograms obtained with different solar telescopes and instrumentation. Existing efforts to characterize these
    Petrie, Gordon J. D. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Cosmology with One Galaxy: Autoencoding the Galaxy Properties Manifold
    Cosmological simulations like CAMELS and IllustrisTNG characterize hundreds of thousands of galaxies using various internal properties. Previous studies have demonstrated that machine learning can be used to infer the cosmological parameter Ω m from the internal properties of even a single randomly selected simulated galaxy. This ability was
    Lue, Amanda et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • The Pristine survey: XXVII. The extremely metal-poor stream C-19 stretches over more than 100 degrees
    The discovery of the most metal-poor stream, C-19, provides us with a fossil record of a stellar structure born very soon after the big bang. In this work, we search for new C-19 members throughout the sky by combining two complementary stream-searching algorithms, STREAMFINDER and StarGO, and utilizing low-metallicity star samples from the
    Yuan, Zhen et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • TOI-6478 b: a cold underdense Neptune transiting a fully convective M dwarf from the thick disc
    Growing numbers of exoplanet detections continue to reveal the diverse nature of planetary systems. Planet formation around late-type M dwarfs is of particular interest. These systems provide practical laboratories to measure exoplanet occurrence rates for M dwarfs, thus testing how the outcomes of planet formation scale with host mass, and how
    Scott, Madison G. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0