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

  • Spectral Indices in the NIR for Studying Stellar Populations
    So far, detailed stellar population studies, based on the absorption line strengths have been concentrated mainly in the optical spectral range. In this work, we supplement spectral indices of the Lick system in the optical with additional indices in the near-infrared (NIR). We optimised the definition of the indices to be sensitive to the main
    Eftekhari, E. et al.

    Fecha de publicación:

    7
    2020
    Número de citas
    0
  • Searching for electromagnetic counterparts to gravitational-wave merger events with the prototype Gravitational-Wave Optical Transient Observer (GOTO-4)
    We report the results of optical follow-up observations of 29 gravitational-wave (GW) triggers during the first half of the LIGO-Virgo Collaboration (LVC) O3 run with the Gravitational-wave Optical Transient Observer (GOTO) in its prototype 4-telescope configuration (GOTO-4). While no viable electromagnetic (EM) counterpart candidate was identified
    Gompertz, B. P. et al.

    Fecha de publicación:

    7
    2020
    Número de citas
    90
  • Revisiting Proxima with ESPRESSO
    Context. The discovery of Proxima b marked one of the most important milestones in exoplanetary science in recent years. Yet the limited precision of the available radial velocity data and the difficulty in modelling the stellar activity calls for a confirmation of the Earth-mass planet. Aims: We aim to confirm the presence of Proxima b using
    Suárez Mascareño, A. et al.

    Fecha de publicación:

    7
    2020
    Número de citas
    105
  • Restoring the night sky darkness at Observatorio del Teide: First application of the model Illumina version 2
    The propagation of artificial light into real environments is complex. To perform its numerical modelling with accuracy, one must consider hyperspectral properties of the lighting devices and their geographic positions, the hyperspectral properties of the ground reflectance, the size and distribution of small-scale obstacles, the blocking effect of
    Aubé, Martin et al.

    Fecha de publicación:

    7
    2020
    Número de citas
    19
  • Radio emission during the formation of stellar clusters in M 33
    Aims: We investigate thermal and nonthermal radio emission associated with the early formation and evolution phases of young stellar clusters (YSCs) selected by their mid-infrared (MIR) emission at 24 μm in M 33. We consider regions in their early formation period, which are compact and totally embedded in the molecular cloud, and in the more
    Corbelli, Edvige et al.

    Fecha de publicación:

    7
    2020
    Número de citas
    1
  • Quenching as a Contest between Galaxy Halos and Their Central Black Holes
    Existing models of galaxy formation have not yet explained striking correlations between structure and star formation activity in galaxies, notably the sloped and moving boundaries that divide star-forming from quenched galaxies in key structural diagrams. This paper uses these and other relations to "reverse engineer" the quenching process for
    Chen, Zhu et al.

    Fecha de publicación:

    7
    2020
    Número de citas
    98