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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  • White Dwarf Binaries across the H-R Diagram
    We created the APOGEE-GALEX-Gaia catalog to study white dwarf (WD) binaries. This database aims to create a minimally biased sample of WD binary systems identified from a combination of GALEX, Gaia, and APOGEE data to increase the number of WD binaries with orbital parameters and chemical compositions. We identify 3414 sources as WD binary
    Anguiano, Borja et al.

    Fecha de publicación:

    10
    2022
    Número de citas
    9
  • Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf
    Context. The NASA space telescope TESS is currently in the extended mission of its all-sky search for new transiting planets. Of the thousands of candidates that TESS is expected to deliver, transiting planets orbiting nearby M dwarfs are particularly interesting targets since they provide a great opportunity to characterize their atmospheres by
    Kawauchi, K. et al.

    Fecha de publicación:

    10
    2022
    Número de citas
    7
  • Ultraviolet Mapping of Polarization Profiles in Chromospheric Plage with CLASP2.1
    Measurement of the magnetic field throughout the solar atmosphere is crucial to a quantitative understanding of energy transfer from the photosphere to the corona, as well as for the dissipation of magnetic energy. However, there remains an overwhelming insufficiency of magnetic measurements in the upper chromosphere and above, where the magnetic
    McKenzie, David et al.

    Fecha de publicación:

    10
    2022
    Número de citas
    0
  • TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star
    The hot Neptune desert is a region hosting a small number of short-period Neptunes in the radius-instellation diagram. Highly irradiated planets are usually either small (R ≲ 2 R ⊕) and rocky or they are gas giants with radii of ≳1 R J. Here, we report on the intermediate-sized planet TOI-2196 b (TIC 372172128.01) on a 1.2 day orbit around a G-type
    Persson, Carina M. et al.

    Fecha de publicación:

    10
    2022
    Número de citas
    15
  • TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley
    We report the discovery and characterization of two small transiting planets orbiting the bright M3.0V star TOI-1468 (LSPM J0106+1913), whose transit signals were detected in the photometric time series in three sectors of the TESS mission. We confirm the planetary nature of both of them using precise radial velocity measurements from the CARMENES
    Chaturvedi, P. et al.

    Fecha de publicación:

    10
    2022
    Número de citas
    18
  • The stable climate of KELT-9b,★
    Even among the most irradiated gas giants, so-called ultra-hot Jupiters, KELT-9b stands out as the hottest planet thus far discovered with a dayside temperature of over 4500 K. At these extreme irradiation levels, we expect an increase in heat redistribution efficiency and a low Bond albedo owed to an extended atmosphere with molecular hydrogen
    Jones, K. et al.

    Fecha de publicación:

    10
    2022
    Número de citas
    16