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

  • Herschel-ATLAS: The angular correlation function of submillimetre galaxies at high and low redshift
    We present measurements of the angular correlation function of galaxies selected from the first field of the H-ATLAS survey. Careful removal of the background from galactic cirrus is essential, and currently dominates the uncertainty in our measurements. For our 250 μm-selected sample we detect no significant clustering, consistent with the
    Maddox, S. J. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    58
  • Herschel-ATLAS: Extragalactic number counts from 250 to 500 microns
    Aims: The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 μm when completed, reaching flux limits (5σ) from 32 to 145 mJy. We here present galaxy number counts obtained for SPIRE
    Clements, D. L. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    109
  • Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5
    We have determined the luminosity function of 250 μm-selected galaxies detected in the ~14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that the luminosity function evolves steadily out to this redshift. By selecting a sub-group of sources within a fixed luminosity
    Dye, S. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    63
  • Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours
    We present colour-colour diagrams of detected sources in the Herschel-ATLAS science demonstration field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies to the spectral energy distribution (SED) to extract the dust temperature of sources with counterparts in Galaxy And Mass Assembly (GAMA) or SDSS surveys with
    Amblard, A. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    123
  • Herschel-ATLAS: Blazars in the science demonstration phase field
    To investigate the poorly constrained sub-mm counts and spectral properties of blazars we searched for these in the Herschel-ATLAS (H-ATLAS) science demonstration phase (SDP) survey catalog. We cross-matched 500 μm sources brighter than 50 mJy with the FIRST radio catalogue. We found two blazars, both previously known. Our study is among the first
    González-Nuevo, J. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    25
  • Herschel unveils a puzzling uniformity of distant dusty galaxies
    The Herschel Space Observatory enables us to accurately measure the bolometric output of starburst galaxies and active galactic nuclei (AGN) by directly sampling the peak of their far-infrared (IR) emission. Here we examine whether the spectral energy distribution (SED) and dust temperature of galaxies have strongly evolved over the last 80% of the
    Elbaz, D. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    190