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

  • Two Transiting Hot Jupiters from the WASP Survey: WASP-150b and WASP-176b
    We report the discovery of two transiting exoplanets from the WASP survey, WASP-150b and WASP-176b. WASP-150b is an eccentric (e = 0.38) hot Jupiter on a 5.6 day orbit around a V = 12.03, F8 main-sequence host. The host star has a mass and radius of 1.4 ${M}_{\odot }$ and 1.7 ${R}_{\odot }$ respectively. WASP-150b has a mass and radius of 8.5 ${M}_
    Cooke, Benjamin F. et al.

    Fecha de publicación:

    6
    2020
    Número de citas
    7
  • The variable radio counterpart of Swift J1858.6-0814
    Swift J1858.6-0814 is a transient neutron star X-ray binary discovered in 2018 October. Multiwavelength follow-up observations across the electromagnetic spectrum revealed many interesting properties, such as erratic flaring on minute time-scales and evidence for wind outflows at both X-ray and optical wavelengths, strong and variable local
    van den Eijnden, J. et al.

    Fecha de publicación:

    6
    2020
    Número de citas
    17
  • The size of galaxies in the era of ultra-deep imaging
    The traditional measurement of the size of galaxies, the effective radius, is a relic of the epoch when shallow imaging was unable to capture the full extension of astronomical sources. However, current deep imaging surveys have revolutionised our view of these objects, allowing us to regard critically our own conventions. In this sense, it is time
    Chamba, N.

    Fecha de publicación:

    6
    2020
    Número de citas
    0
  • The SDSS/APOGEE catalogue of HgMn stars
    We report on H-band spectra of chemically peculiar Mercury-Manganese (HgMn) stars obtained via the SDSS/APOGEE survey. As opposed to other varieties of chemically peculiar stars such as classical Ap/Bp stars, HgMn stars lack strong magnetic fields and are defined by extreme overabundances of Mn, Hg, and other heavy elements. A satisfactory
    Chojnowski, S. Drew et al.

    Fecha de publicación:

    6
    2020
    Número de citas
    19
  • The SAMI Galaxy Survey: Stellar Population Gradients of Central Galaxies
    We examine the stellar population radial gradients (age, metallicity, and [α/Fe]) of 96 passive central galaxies up to ∼2 R e in the SAMI Galaxy Survey. The targeted groups have a halo mass range of $11\lt \mathrm{log}({M}_{200}/{M}_{\odot })\lt 15$ . The main goal of this work is to determine whether central galaxies have different stellar
    Santucci, Giulia et al.

    Fecha de publicación:

    6
    2020
    Número de citas
    34
  • The nature of 500 micron risers I: SMA observations
    We present SMA observations at resolutions from 0.35 to 3 arcsec of a sample of 34 candidate high redshift dusty star forming galaxies (DSFGs). These sources were selected from the HerMES Herschel survey catalogues to have SEDs rising from 250 to 350 to 500 μm, a population termed 500-risers. We detect counterparts to 24 of these sources, with four
    Greenslade, J. et al.

    Fecha de publicación:

    6
    2020
    Número de citas
    12