Astrophysical: Star formation

  • Publication
    Stellar mass-metallicity relation throughout the large-scale structure of the Universe: CAVITY mother sample
    Context. Void galaxies are essential for understanding the physical processes that drive galaxy evolution because they are less affected by external factors...
  • Publication
    Stellar masses of giant clumps in CANDELS and simulated galaxies using machine learning
    A significant fraction of high redshift star-forming disc galaxies are known to host giant clumps, whose nature and role in galaxy evolution are yet to be...
  • Publication
    Stellar masses of star-forming galaxies at 0.3 < z < 1.2 in the GOYA survey
    Starforming galaxies with compact morphology and high optical luminosity (LBCGs) are very common at redshitfs z = 0.4 - 1.2. Those galaxies are believed to have...
  • Publication
    Stellar Population Synthesis of Star-forming Clumps in Galaxy Pairs and Non-interacting Spiral Galaxies
    We have identified 1027 star-forming complexes in a sample of 46 galaxies from the Spirals, Bridges, and Tails (SB&T) sample of interacting galaxies, and 693...
  • Publication
    Stellar populations across galaxy bars in the MUSE TIMER project
    Stellar populations in barred galaxies save an imprint of the influence of the bar on the host galaxy's evolution. We present a detailed analysis of star...
  • Publication
    Stellar populations in interacting systems of the Second Byurakan Survey
    We have started an observing program to study the whole sample of interaction systems from the Second Byurakan Survey (SBS) (around 20 sky fields) using a CCD...
  • Publication
    Stellar populations of early-type galaxies in the ATLAS3D sample
    ATLAS3D is a multi-wavelength, volume-limited survey of 263 morphologically-selected early-type galaxies within a distance of 42 Mpc and complete to MK
  • Publication
    Strategies for AGN characterisation in the OTELO survey
    We present the current status of definition of the observational and analysis strategies for the study of Active Galactic Nuclei (AGN) in the OTELO survey. The...
  • Publication
    Strong size evolution of disc galaxies since z = 1. Readdressing galaxy growth using a physically motivated size indicator
    Our understanding of how the size of galaxies has evolved over cosmic time is based on the use of the half-light (effective) radius as a size indicator...