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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  • Discovery of an Ultra-diffuse Galaxy in the Pisces--Perseus Supercluster
    We report the discovery of DGSAT I, an ultra-diffuse, quenched galaxy located 10.°4 in projection from the Andromeda galaxy (M31). This low-surface brightness galaxy (μV = 24.8 mag arcsec‑2), found with a small amateur telescope, appears unresolved in sub-arcsecond archival Subaru/Suprime-Cam images, and hence has been missed by optical surveys
    Martínez-Delgado, D. et al.

    Fecha de publicación:

    4
    2016
    Número de citas
    131
  • Discovery of a massive supercluster system at z ~ 0.47
    Aims: Superclusters are the largest relatively isolated systems in the cosmic web. Using the SDSS BOSS survey, we search for the largest superclusters in the redshift range 0.43 z 0.71. Methods: We generate a luminosity-density field smoothed over 8 h-1Mpc to detect the large-scale over-density regions. Each individual over-density region is
    Lietzen, H. et al.

    Fecha de publicación:

    4
    2016
    Número de citas
    38
  • Design concepts and options for the Thermal Infrared Imager (TIRI) as part of ESA's Asteroid Impact Mission.
    ESA's Asteroid Impact Mission (AIM) is being studied as part of the joint ESA/NASA AIDA mission for launch in 2020. AIDA's primary mission is to investigate the effect of a kinetic impactor on the secondary component of the binary asteroid 65803 Didymos in late 2022. AIM will characterise the Didymos system and monitor the response of the binary
    Bowles, Neil et al.

    Fecha de publicación:

    4
    2016
    Número de citas
    0
  • Departure from the constant-period ephemeris for the transiting exoplanet WASP-12
    Aims: Most hot Jupiters are expected to spiral in toward their host stars because the angular momentum of the orbital motion is transferred to the stellar spin. Their orbits can also precess as a result of planet-star interactions. Calculations show that both effects might be detected for the very-hot exoplanet WASP-12 b using the method of precise
    Maciejewski, G. et al.

    Fecha de publicación:

    4
    2016
    Número de citas
    130
  • Chemical history of isolated dwarf galaxies of the Local Group - I. dSphs: Cetus and Tucana
    For the first time, we obtain chemical evolution models (CEMs) for Tucana and Cetus, two isolated dwarf spheroidal galaxies of the Local Group. The CEMs have been built from the star formation histories (SFHs) and the metallicity histories, both obtained independently by the Local Cosmology from Isolated Dwarfs (LCID) project from deep colour
    Avila-Vergara, N. et al.

    Fecha de publicación:

    4
    2016
    Número de citas
    5
  • Carbon stars in the X-Shooter Spectral Library⋆⋆⋆
    We provide a new collection of spectra of 35 carbon stars obtained with the ESO/VLT X-Shooter instrument as part of the X-Shooter Spectral Library project. The spectra extend from 0.3 μm to 2.4 μm with a resolving power above ~8000. The sample contains stars with a broad range of (J - K) color and pulsation properties located in the Milky Way and
    Gonneau, A. et al.

    Fecha de publicación:

    4
    2016
    Número de citas
    33