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

  • LIRIS Multi-slit Hα Spectroscopy of a z˜1 DEEP2 Sample of Star-forming Galaxies
    We present preliminary results of Hα near-infrared spectroscopy of six galaxies with redshifts z˜1 drawn from the DEEP2 Galaxy Redshift Survey. The spectra have been taken with the multi-object mode of LIRIS (Long-slit Intermediate Resolution Infrared Spectrograph) installed at the 4.2-m William Herschel Telescope. This is a pilot study for a
    Rodríguez-Eugenio, N. et al.

    Fecha de publicación:

    3
    2008
    Número de citas
    0
  • IPHAS and the symbiotic stars. I. Selection method and first discoveries
    Context: The study of symbiotic stars is essential to understand important aspects of stellar evolution in interacting binaries. Their observed population in the Galaxy is however poorly known, and is one to three orders of magnitudes smaller than the predicted population size. Aims: IPHAS, the INT Photometric Hα survey of the Northern Galactic
    Corradi, R. L. M. et al.

    Fecha de publicación:

    3
    2008
    Número de citas
    120
  • Infrared Constraints on AGN Tori Models
    This work focuses on the properties of dusty tori in active galactic nuclei (AGN) derived from the comparison of SDSS type 1 quasars with mid-Infrared (MIR) counterparts and a new, detailed torus model. The infrared data were taken by the Spitzer Wide-area InfraRed Extragalactic (SWIRE) Survey. Basic model parameters are constraint, such as the
    Hatziminaoglou, E. et al.

    Fecha de publicación:

    3
    2008
    Número de citas
    1
  • Geometry Diagnostics of a Stellar Flare from Fluorescent X-Rays
    We present evidence of Fe fluorescent emission in the Chandra HETGS spectrum of the single G-type giant HR 9024 during a large flare. In analogy to solar X-ray observations, we interpret the observed Fe Kα line as being produced by illumination of the photosphere by ionizing coronal X-rays, in which case, for a given Fe photospheric abundance, its
    Testa, Paola et al.

    Fecha de publicación:

    3
    2008
    Número de citas
    23
  • Gemini/GMOS spectroscopy of the spheroid and globular cluster system of NGC 3923
    We present a technique to extract ultra-deep diffuse-light spectra from the standard multi-object spectroscopic observations used to investigate extragalactic globular cluster (GC) systems. This technique allows a clean extraction of the spectrum of the host galaxy diffuse light from the same slitlets as the GC targets. We show the utility of the
    Norris, Mark A. et al.

    Fecha de publicación:

    3
    2008
    Número de citas
    52
  • Galaxy Counts at 24 μm in the SWIRE Fields
    This paper presents galaxy source counts at 24 μm in the six Spitzer Wide-field InfraRed Extragalactic (SWIRE) fields. The source counts are compared to counts in other fields, and to model predictions that have been updated since the launch of Spitzer. This analysis confirms a very steep rise in the Euclidean-normalized differential number counts
    Shupe, David L. et al.

    Fecha de publicación:

    3
    2008
    Número de citas
    53