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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  • The mechanical design for the WEAVE prime focus corrector system
    WEAVE is the next-generation, wide-field, optical spectroscopy facility for the William Herschel Telescope (WHT) in La Palma, Canary Islands, Spain. The WHT will undergo a significant adaptation to accommodate this facility. A two- degree Prime Focus Corrector (PFC), that includes an Atmospheric Dispersion Compensator, is being planned and is
    Abrams, D. C. et al.

    Fecha de publicación:

    8
    2014
    Número de citas
    3
  • The innermost globular clusters of M87
    We present a comprehensive multiwavelength photometric analysis of the innermost (˜3 × 3 kpc2) 110 globular clusters (GCs) of M87. Their spectral energy distributions (SEDs) were built taking advantage of new ground-based high-resolution near-infrared imaging aided by adaptive optics at the Very Large Telescope combined with Hubble Space Telescope
    Montes, M. et al.

    Fecha de publicación:

    8
    2014
    Número de citas
    12
  • The impact of galaxy formation on the total mass, mass profile and abundance of haloes
    We use cosmological hydrodynamical simulations to investigate how the inclusion of physical processes relevant to galaxy formation (star formation, metal-line cooling, stellar winds, supernovae and feedback from active galactic nuclei, AGN) change the properties of haloes, over four orders of magnitude in mass. We find that gas expulsion and the
    Velliscig, M. et al.

    Fecha de publicación:

    8
    2014
    Número de citas
    175
  • The halo+cluster system of the Galactic globular cluster NGC 1851
    NGC 1851 is surrounded by a stellar component that extends more than 10 times beyond the tidal radius. Although the nature of this stellar structure is not known, it has been suggested to be a sparse halo of stars or associated with a stellar stream. We analyse the nature of this intriguing stellar component surrounding NGC 1851 by investigating
    Marino, A. F. et al.

    Fecha de publicación:

    8
    2014
    Número de citas
    67
  • The Gaia-ESO Survey: Metallicity of the Chamaeleon I star-forming region
    Context. Recent metallicity determinations in young open clusters and star-forming regions suggest that the latter may be characterized by a slightly lower metallicity than the Sun and older clusters in the solar vicinity. However, these results are based on small statistics and inhomogeneous analyses. The Gaia-ESO Survey is observing and
    Spina, L. et al.

    Fecha de publicación:

    8
    2014
    Número de citas
    43
  • The control unit of the near infrared spectrograph of the EUCLID space mission: preliminary design
    The Near Infrared Spectrograph and Photometer (NISP) is one of the instruments on board the ESA EUCLID mission. The Universidad Politecnica de Cartagena and Instituto de Astrofisica de Canarias are responsible of the Instrument Control Unit of the NISP (NI-ICU) in the Euclid Consortium. The NI-ICU main functions are: communication with the S/C and
    Toledo-Moreo, R. et al.

    Fecha de publicación:

    8
    2014
    Número de citas
    1