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

  • High spatial resolution and high contrast optical speckle imaging with FASTCAM at the ORM
    In this paper, we present an original observational approach, which combines, for the first time, traditional speckle imaging with image post-processing to obtain in the optical domain diffraction-limited images with high contrast (10-5) within 0.5 to 2 arcseconds around a bright star. The post-processing step is based on wavelet filtering an has
    Labadie, L. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    0
  • Herschel-SPIRE observations of the disturbed galaxy NGC 4438
    We present Herschel-SPIRE observations of the perturbed galaxy NGC 4438 in the Virgo cluster. These images reveal the presence of extra-planar dust up to ~4-5 kpc away from the galaxy's disk. The dust closely follows the distribution of the stripped atomic and molecular hydrogen, supporting the idea that gas and dust are perturbed in a similar
    Cortese, L. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    31
  • Herschel-ATLAS: The dust energy balance in the edge-on spiral galaxy UGC 4754
    We use Herschel PACS and SPIRE observations of the edge-on spiral galaxy UGC 4754, taken as part of the H-ATLAS SDP observations, to investigate the dust energy balance in this galaxy. We build detailed SKIRT radiative models based on SDSS and UKIDSS maps and use these models to predict the far-infrared emission. We find that our radiative transfer
    Baes, M. et al.

    Fecha de publicación:

    7
    2010
    Número de citas
    87
  • 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
    57
  • 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
    107
  • 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