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 dynamical state of bars in cluster dwarf galaxies: the cases of NGC 4483 and NGC 4516

    Dwarf barred galaxies are the perfect candidates for hosting slowly rotating bars. They are common in dense environments and have a relatively shallow potential well, making them prone to heating by interactions. When an interaction induces bar formation, the bar should rotate slowly. They reside in massive and centrally concentrated dark matter

    Cuomo, Virginia et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    0
  • TOI-544 b: a potential water-world inside the radius valley in a two-planet system

    We report on the precise radial velocity follow-up of TOI-544 (HD 290498), a bright K star (V = 10.8), which hosts a small transiting planet recently discovered by the Transiting Exoplanet Survey Satellite (TESS). We collected 122 high-resolution High Accuracy Radial velocity Planet Searcher (HARPS) and HARPS-N spectra to spectroscopically confirm

    Osborne, H. L. M. et al.

    Fecha de publicación:

    2
    2024
    Número de citas
    0
  • Catalogue of BRITE-Constellation targets. I. Fields 1 to 14 (November 2013-April 2016)

    Context. The BRIght Target Explorer (BRITE) mission collects photometric time series in two passbands with the aim of investigating stellar structure and evolution. Since their launches in the years 2013 and 2014, the constellation of five BRITE nano-satellites has observed a total of more than 700 individual bright stars in 64 fields. Some targets

    Zwintz, K. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • Characterising the intra-cluster light in The Three Hundred simulations

    We characterise the intra-cluster light (ICL) in ensembles of full-physics cluster simulations from THE THREE HUNDRED project, a suite of 324 hydrodynamical resimulations of cluster-sized halos. We identify the ICL as those stellar particles bound to the potential of the cluster itself, but not to any of its substructures, and separate the

    Contreras-Santos, A. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • Characterizing the ELG luminosity functions in the nearby Universe

    Context. Nebular emission lines are powerful diagnostics for the physical processes at play in galaxy formation and evolution. Moreover, emission-line galaxies (ELGs) are one of the main targets of current and forthcoming spectroscopic cosmological surveys. Aims: We investigate the contributions to the line luminosity functions (LFs) of different

    Favole, G. et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0
  • Extremely Red Galaxies at z = 5–9 with MIRI and NIRSpec: Dusty Galaxies or Obscured Active Galactic Nuclei?

    We study a new population of extremely red objects (EROs) recently discovered by the James Webb Space Telescope (JWST) based on their NIRCam colors F277W ‑ F444W > 1.5 mag. We find 37 EROs in the Cosmic Evolution Early Release Science Survey (CEERS) field with F444W < 28 mag and photometric redshifts between 5 < z < 7, with median $z={6.9}_{-1.6}^{

    Barro, Guillermo et al.

    Fecha de publicación:

    3
    2024
    Número de citas
    0