Astrofísicas: Galaxias

  • Publicación
    The Evolution of Passive Galaxies since z=1: Major Mergers vs Secular Processes
    We study the evolution of the red sequence and the blue cloud since z ~ 1 to present in GOODS-S field for MB ≤ -20 and M* ≥ 1010 M&sun; selected galaxies. We...
  • Publicación
    The evolution of quiescent galaxies at high redshifts (z≥ 1.4)
    The goal of this work is to study the evolution of high-redshift (z≥ 1.4) quiescent galaxies over an effective area of ˜1.7 deg2 in the COSMOS field. Galaxies...
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    The evolution of rest-frame UV properties, Ly α EWs, and the SFR-stellar mass relation at z ̃ 2-6 for SC4K LAEs
    We explore deep rest-frame UV to FIR data in the COSMOS field to measure the individual spectral energy distributions (SED) of the ̃4000 SC4K (Sobral et al.)...
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    The Evolution of Spiral, S0, and Elliptical Galaxies in Clusters
    We quantify the evolution of the spiral, S0 and elliptical fractions in galaxy clusters as a function of cluster velocity dispersion (σ) and X-ray luminosity...
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    The evolution of the dust temperatures of galaxies in the SFR-M∗ plane up to z s 2
    We study the evolution of the dust temperature of galaxies in the SFR- M∗ plane up to z ~ 2 using far-infrared and submillimetre observations from the Herschel...
  • Publicación
    The Evolution of the Number Density of Compact Galaxies
    We compare the number density of compact (small size) massive galaxies at low and high redshift using our Padova Millennium Galaxy and Group Catalogue (PM2GC)...
  • Publicación
    The evolution of the UV luminosity and stellar mass functions of Lyman-α emitters from z 2 to z 6
    We measure the evolution of the rest-frame UV luminosity function (LF) and the stellar mass function (SMF) of Lyman-α (Ly α) emitters (LAEs) from z ~ 2 to z ~ 6...
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    The evolution of the UV/optical lag spectrum of NGC 7469 seen by the Liverpool Telescope
    We present the results regarding the analysis of an intensive monitoring of the Active Galactic Nucleus (AGN) NGC 7469. We observed the source for 4 months with...
  • Publicación
    The evolution of ultra-diffuse galaxies in nearby galaxy clusters from the Kapteyn IAC WEAVE INT Clusters Survey
    We study the population of ultra-diffuse galaxies (UDGs) in a set of eight nearby (z 0.035) galaxy clusters, from the Kapteyn IAC WEAVE INT Clusters Survey. We...