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: v1.2.3
    Minor bug fix release. See the changelog for details.
    Koposov, Sergey et al.

    Fecha de publicación:

    6
    2022
    Número de citas
    15
  • Fitting of supernovae without dark energy
    With data from Pantheon, we have at our disposal a sample of more than a 1000 supernovae Ia covering a wide range of redshifts with good precision. Here, we make fits to the corresponding Hubble-Lemaître diagram with various cosmological models, with intergalactic extinction, evolution of the luminosity of supernovae, and redshift components due to
    López-Corredoira, M. et al.

    Fecha de publicación:

    8
    2022
    Número de citas
    6
  • The ultraviolet researcher to investigate the emergence of life: a mission proposal to ESA's F-call
    The mission Ultraviolet Researcher to Investigate the Emergence of Life (URIEL) is designed to carry out low dispersion (600-1,000) UV spectropolarimetry in the 140-400 nm spectral range to investigate the formation of planetary systems, its interaction with stellar winds and search for signatures of prebiotic molecules by remote sensing of small
    Gómez de Castro, Ana I. et al.

    Fecha de publicación:

    8
    2022
    Número de citas
    0
  • Density, not radius, separates rocky and water-rich small planets orbiting M dwarf stars
    Exoplanets smaller than Neptune are common around red dwarf stars (M dwarfs), with those that transit their host star constituting the bulk of known temperate worlds amenable for atmospheric characterization. We analyze the masses and radii of all known small transiting planets around M dwarfs, identifying three populations: rocky, water-rich, and
    Luque, Rafael et al.

    Fecha de publicación:

    9
    2022
    Número de citas
    141
  • A dense 0.1-solar-mass star in a 51-minute-orbital-period eclipsing binary
    Of more than a thousand known cataclysmic variables (CVs), where a white dwarf is accreting from a hydrogen-rich star, only a dozen have orbital periods below 75 minutes 1-9. One way to achieve these short periods requires the donor star to have undergone substantial nuclear evolution before interacting with the white dwarf 10-14, and it is
    Burdge, Kevin B. et al.

    Fecha de publicación:

    10
    2022
    Número de citas
    10