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

  • Witnessing the rapid growth of disk galaxies over cosmic time
    The Hubble and James Webb Space Telescopes, with their outstanding depth and spatial resolution, are opening up the possibility of studying the edges of disk galaxies over a significant cosmic time interval. This allows us to study in detail the evolution of galaxy edges over the past 8 Gyr. The edge of galaxies, understood here as the farthest
    Raji, Samane et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • Using gas kinematics to measure resonant structures in disc galaxies: the interaction of M51 with NGC 5195
    Interstellar gas offers advantages when quantifying the structure of the resonances in disc galaxies. The gas is concentrated close to the disc mid-plane, making it easier to determine its in-plane velocity components, and it offers sharp emission lines for good velocity resolution. These properties are shared by atomic, molecular, and ionized gas
    Beckman, John et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • Using autoencoders and deep transfer learning to determine the stellar parameters of 286 CARMENES M dwarfs
    Context. Deep learning (DL) techniques are a promising approach among the set of methods used in the ever-challenging determination of stellar parameters in M dwarfs. In this context, transfer learning could play an important role in mitigating uncertainties in the results due to the synthetic gap (i.e. difference in feature distributions between
    Mas-Buitrago, P. et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    2
  • Use of a finite state machine approach for sequence control in the GREGOR infrared spectrograph (GRIS)
    Due to the complexity of scientific instruments, such as spectropolarimeters, managing instrument sequences can be challenging. To address this problem, a Finite-State Machine (FSM) approach has been used to manage solar observation sequences in the GREGOR Infrared Spectrograph (GRIS). FSMs provide a structured and visual representation of control
    Matta-Gómez, A. et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • Unveiling the central kpc of Type I AGN host galaxies in seeing-limited IFS data
    The evolution of galaxies appears linked to the growth of supermassive black holes (SMBH), as evidenced by empirical scale relations between hosts' large-scale properties and the mass of their central black holes. This co-evolutionary scenario suggests that all galaxies experience nuclear activity — active phases during which the black hole
    García Lorenzo, Begoña et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • Unveiling the (in)consistencies among the galaxy stellar mass function, star formation histories, satellite abundances, and intracluster light from a semi-empirical perspective
    In a hierarchical, dark matter-dominated Universe, stellar mass functions (SMFs), galaxy merger rates, star formation histories (SFHs), satellite abundances, and intracluster light (ICL), should all be intimately connected observables. However, the systematics affecting observations still prevent universal and uniform measurements of, for example
    Fu, Hao et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    4