Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • Herschel FIR counterparts of selected Lyα emitters at z ~ 2.2. Fast evolution since z ~ 3 or missed obscured AGNs?
    Lyα emitters (LAEs) are seen everywhere in the redshift domain from local to z ~ 7. Far-infrared (FIR) counterparts of LAEs at different epochs could provide direct clues on dust content, extinction, and spectral energy distribution (SED) for these galaxies. We search for FIR counterparts of LAEs that are optically detected in the GOODS-North field
    Bongiovanni, A. et al.

    Advertised on:

    9
    2010
    Citations
    19
  • Galaxy morphology in 5 medium redshift clusters (Ascaso+, 2009)
    Following the study presented in our previous paper, based on the Nordic Optical Telescope (NOT) sample, which consists of five clusters of galaxies within the redshift range 0.18
    Ascaso, B. et al.

    Advertised on:

    9
    2010
    Citations
    0
  • Galactic evolution of oxygen. OH lines in 3D hydrodynamical model atmospheres
    Context. Oxygen is the third most common element in the Universe. The measurement of oxygen lines in metal-poor unevolved stars, in particular near-UV OH lines, can provide invaluable information about the properties of the Early Galaxy. Aims: Near-UV OH lines constitute an important tool to derive oxygen abundances in metal-poor dwarf stars
    González Hernández, J. I. et al.

    Advertised on:

    9
    2010
    Citations
    35
  • EVOLUCIÓN QUÍMICA DE GALAXIAS UTILIZANDO EL SDSS
    Premio Extraordinario de Doctorado 2010
    MARITZA ARLENE LARA LÓPEZ

    Advertised on:

    9
    2010
  • Detection of frequency spacings in the young O-type binary HD 46149 from CoRoT photometry
    Aims: Using the CoRoT space based photometry of the O-type binary HD 46149, stellar atmospheric effects related to rotation can be separated from pulsations, because they leave distinct signatures in the light curve. This offers the possibility of characterising and exploiting any pulsations seismologically. Methods: Combining high-quality space
    Degroote, P. et al.

    Advertised on:

    9
    2010
    Citations
    59