Astrophysical: Galaxies

  • Publication
    Ks Number Counts in the Groth and Coppi Fields
    We have used William Herschel Telescope/INGRID Ks images on two high-latitude fields, the Coppi and Groth strips, to obtain galaxy number counts over ~180...
  • Publication
    K[s] number counts in the Groth and Coppi fields
    The COSMOS Survey is currently mapping 0.5 deg2 of sky in optical and near-IR bands to definesamples of compact galaxies at high redshift for spectroscopic...
  • News
    La investigadora del IAC Casiana Muñoz, galardonada con la Medalla de Andalucía
    La astrofísica cordobesa Casiana Muñoz Tuñón ha sido distinguida con la Medalla de Andalucía en la categoría de Investigación, Ciencia y Salud, un...
  • Publication
    LAEs & LBGs with OSIRIS
    We present preliminary results of an on going program to study Lyman Alpha Emitters, Lyman Break Galaxies, and Quasars at high redshift with the OSIRIS...
  • Publication
    Large Disklike Galaxies at High Redshift
    Using deep near-infrared imaging of the Hubble Deep Field-South with the Infrared Spectrometer and Array Camera on the Very Large Telescope, we find six large...
  • Publication
    Large Scale Absorbers in the Environment of High-z Radio-Galaxies
    We discuss a number of interesting questions that arise from studies of extended absorbers observed in high redshift radio-galaxies. We propose to carry out 2-D...
  • Publication
    Large-scale environments of z < 0.4 active galaxies
    Context. Properties of galaxies depend on their large-scale environment. As the influence of active galactic nuclei (AGN) in galaxy evolution is becoming more...
  • Publication
    Large-scale stellar age-velocity spiral pattern in NGC 4030
    The processes driving the formation and evolution of late-type galaxies continue to be a debated subject in extragalactic astronomy. Investigating stellar...
  • Publication
    Larger λ<SUB>R</SUB> in the disc of isolated active spiral galaxies than in their non-active twins
    We present a comparison of the spin parameter λ R, measured in a region dominated by the galaxy disc, between 20 pairs of nearby (0.005 < z < 0.03) seemingly...