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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  • Educational Project with Robotic Telescopes (PETeR): robots looking to the future
    The ``Proyecto Educativo con Telescopios Robóticos'' (PETeR) of the Instituto de Astrofísica de Canarias is an online inquiry-based laboratory that allows school students to carry out their own observations and research projects in astronomy using professional robotic telescopes. The availability of observing time on several telescopes, which also
    Rodríguez Eugenio, N.

    Fecha de publicación:

    5
    2023
    Número de citas
    1
  • Do machines dream of modelling AGB stars?
    It is very common in astrophysics that certain relevant parameters of the objects studied cannot be obtained directly from observations, but require numerical models that simulate the relevant physical mechanisms, often through an iterative process of trial and error. This is often lengthy and consumes a large part of the human and material
    Santander-García, M. et al.

    Fecha de publicación:

    5
    2023
    Número de citas
    0
  • Discovery of a substellar companion in the TESS light curve of the δ Scuti/γ Doradus hybrid pulsator HD 31221
    Context. Close-in, sub-stellar companions to δ Scuti type stars present a highly suitable testbed for examining how planetary-mass objects can influence stellar pulsations. Aims: We aim to constrain the mass of HD 31221 b, probe its atmosphere, and demonstrate how it affects the pulsational pattern of its host, HD 31221. Methods: We made use of the
    Kálmán, Sz. et al.

    Fecha de publicación:

    5
    2023
    Número de citas
    5
  • Detection of Carbon Monoxide's 4.6 Micron Fundamental Band Structure in WASP-39b's Atmosphere with JWST NIRSpec G395H
    Carbon monoxide (CO) is predicted to be the dominant carbon-bearing molecule in giant planet atmospheres and, along with water, is important for discerning the oxygen and therefore carbon-to-oxygen ratio of these planets. The fundamental absorption mode of CO has a broad, double-branched structure composed of many individual absorption lines from 4
    Grant, David et al.

    Fecha de publicación:

    5
    2023
    Número de citas
    16
  • Detection of a high-velocity sodium feature on the ultra-hot Jupiter WASP-121 b
    Context. Ultra-hot Jupiters, with their high equilibrium temperatures and resolved spectral lines, have emerged as a perfect testbed for new analysis techniques in the study of exoplanet atmospheres. In particular, the resolved sodium doublet as a resonant line has proven a powerful indicator to probe the atmospheric structure over a wide pressure
    Seidel, J. V. et al.

    Fecha de publicación:

    5
    2023
    Número de citas
    24
  • DESI mock challenge. Halo and galaxy catalogues with the bias assignment method
    Context. We present a novel approach to the construction of mock galaxy catalogues for large-scale structure analysis based on the distribution of dark matter halos obtained with effective bias models at the field level. Aims: We aim to produce mock galaxy catalogues capable of generating accurate covariance matrices for a number of cosmological
    Balaguera-Antolínez, Andrés et al.

    Fecha de publicación:

    5
    2023
    Número de citas
    15