Publication type: Non-refereed

  • Publication
    Quantification of bar strength and the structure of galaxies
    Not Available
  • Publication
    Quantifying downsizing & its origin: the mass assembly of galaxies and the role of AGN
    We present our latest results based on the Spitzer Cosmological Surveys about the characterization of the mass assembly of galaxies in the last 12 Gyr. We have...
  • Publication
    Quantifying high z galaxy selection and visibility with the COSMOPACK tool
    We have developed COSMOPACK, a set of tools that transform images of real galaxies to depict their appearance at a given redshift as observed with a given...
  • Publication
    Quantifying the ionising flux escaping from the ultra-luminous HII regions in four spiral galaxies
    There are two principal problems in explaining, in terms of the emission from OB stars, the ionisation of the gas which emits the diffuse H-alpha in spiral...
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    Quantifying the typical scale of star formation in the spiral arms through their young stellar clusters
    Star formation is a vital phenomenon across all fields of astronomy, shaping our universe in all its vastness, from the small scale of exoplanets to the large...
  • Publication
    Quantitative Galaxy Morphology of Five Medium Redshift Clusters
    We have studied the quantitative morphology and structural parameters of the bright galaxy population in the Nordic Optical Telescope (NOT) sample, which...
  • Publication
    Quantitative Morphological Analysis of Galaxies at Intermediate Red Shift: Clues to Galaxy Evolution
    We have developed morphological analysis software for studying galaxies from low to high redshifts. This code is designed to extract quantitative information...
  • Publication
    Quantitative Morphology of Galaxies at Medium Redshift: Abell Cluster 2443
    First results of a photometric study of the richness=2 Abell Cluster 2443 at z=0.103 are presented. We have developed a new algorithm to perform a detailed...
  • Publication
    Quantitative spectroscopic analyses in the IACOB+OWN project: Massive O-type stars in the Galaxy with the current Gaia information
    We present the results from the quantitative spectroscopic analysis of ~280 likely single O stars targeted by the IACOB and OWN surveys. This implies the...