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

  • joshspeagle/dynesty: v2.1.0
    This a major release with a significant change of the sampler. It is now able to correctly sample likelihood functions with plateaus, (i.e likelihood functions with areas where likelihood value is exactly the same). The previous behaviour also led to inaccurate log(Z) estimates if some fraction of the prior volume had log(P)=-LARGENUMBER
    Koposov, Sergey et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    16
  • JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334
    We study the HII regions associated with the NGC 6334 molecular cloud observed in the submillimeter and taken as part of the B-fields In STar-forming Region Observations Survey. In particular, we investigate the polarization patterns and magnetic field morphologies associated with these HII regions. Through polarization pattern and pressure
    Li, Di et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    21
  • Impact of opacity effects on chromospheric oscillations inferred from NLTE inversions
    Context. Spectropolarimetric inversions are a fundamental tool for diagnosing the solar atmosphere. Chromospheric inferences rely on the interpretation of spectral lines that are formed under nonlocal thermodynamic equilibrium (NLTE) conditions. In the presence of oscillations, changes in the opacity impact the response height of the spectral lines
    Felipe, T. et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    5
  • Identification of carbon dioxide in an exoplanet atmosphere
    Carbon dioxide (CO 2) is a key chemical species that is found in a wide range of planetary atmospheres. In the context of exoplanets, CO 2 is an indicator of the metal enrichment (that is, elements heavier than helium, also called `metallicity') 1-3, and thus the formation processes of the primary atmospheres of hot gas giants 4-6. It is also one
    JWST Transiting Exoplanet Community Early Release Science Team et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    188
  • Exploring Magnetic Loops and Serpentine Fields in the Quiet Sun with the GRIS-IFU
    Synthetic observations produced from radiative magnetohydrodynamic simulations have predicted that higher polarization fractions in the quiet solar photosphere would be revealed by increasing the total integration time of observations at GREGOR resolutions. We present recently acquired disk center observations of the Fe I 15648.5 Å line obtained
    Collados, Manuel et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    3
  • Evolution of dark gaps in barred galaxies
    Context. Recent studies show that barred galaxies have a light deficit, called a dark gap (DG), in the direction of the bar minor axis with respect to the major axis. The properties of these DGs might be related to the properties of the bars and to the location of some resonances of the galaxies. Aims: We have analyzed the evolution of the DGs
    Aguerri, J. A. L. et al.

    Fecha de publicación:

    2
    2023
    Número de citas
    3