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..

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  • The co-evolution of strong AGN and central galaxies in different environments
    We exploit a sample of 80 000 Sloan Digital Sky Survey central galaxies to investigate the effect of active galactic nucleus (AGN) feedback on their evolution. We trace the demographics of optically selected AGN (Seyferts) as a function of their internal properties and environment. We find that the preeminence of AGN as the dominant ionizing
    Sampaio, V. M. et al.

    Fecha de publicación:

    10
    2023
    Número de citas
    3
  • The nature of the X-ray sources in dwarf galaxies in nearby clusters from the KIWICS
    We present a deep search for and analysis of X-ray sources in a sample of dwarf galaxies (M r < -15.5 mag) located within twelve galaxy clusters from the Kapteyn IAC WHT Enhanced Area Velocity Explores Isaac Newton Telescope Cluster Survey of photometric observations in the r and g using the Wide Field Camera at the 2.5-m Isaac Newton telescope. We
    Şen, Şeyda et al.

    Fecha de publicación:

    10
    2023
    Número de citas
    0
  • The PSZ-MCMF catalogue of Planck clusters over the DES region
    We present the first systematic follow-up of Planck Sunyaev-Zeldovich effect (SZE) selected candidates down to signal-to-noise (S/N) of 3 over the 5000 deg 2 covered by the Dark Energy Survey. Using the MCMF cluster confirmation algorithm, we identify optical counterparts, determine photometric redshifts, and richnesses and assign a parameter, f
    Hernández-Lang, D. et al.

    Fecha de publicación:

    10
    2023
    Número de citas
    10
  • Ultra diffuse galaxies in the Hydra I cluster from the LEWISProject: Phase-Space distribution and globular cluster richness
    Although ultra diffuse galaxies (UDGs) are found in large numbers in clusters of galaxies, the role of the cluster environment in shaping their low surface brightness and large sizes is still uncertain. Here, we examine a sample of UDGs in the Hydra I cluster (D = 51 Mpc) with new radial velocities obtained as part of the LEWIS (Looking into the
    Forbes, Duncan A. et al.

    Fecha de publicación:

    10
    2023
    Número de citas
    6
  • COSMOLOGICAL BAYESIAN INFERENCE IN HIGH DIMENSIONAL SPACES
    The different structures we observe in the Universe result from cosmic evolution starting from primordial seeds. These are believed to have originated from quantum fluctuations. During the inflationary epoch, they were stretched and frozen just after the Big Bang, giving rise to an almost homogeneous, closely Gaussian-distributed Universe. However
    Mónica Hernández Sánchez

    Fecha de publicación:

    5
    2023
  • Galaxies in voids assemble their stars slowly
    Galaxies in the Universe are distributed in a web-like structure characterized by different large-scale environments: dense clusters, elongated filaments, sheetlike walls and under-dense regions, called voids 1-5. The low density in voids is expected to affect the properties of their galaxies. Indeed, previous studies 6-14 have shown that galaxies
    Domínguez-Gómez, Jesús et al.

    Fecha de publicación:

    7
    2023
    Número de citas
    12