Kate Rowlands

     

    Main Research Fields

    • Galaxy transformation - starbursts, galaxy mergers, post-starburst galaxies, quenching
    • Connection between galaxy morphology and physical properties
    • Multiwavelength spectral energy distribution (SED) modelling
    • Large multiwavelength surveys
    • Integral field spectroscopy
    • Properties, origins and evolution of dust and gas in galaxies

    Keywords

    • Galaxy formation and evolution
    • Mass functions, Luminosity functions, Star formation rates, Stellar masses, Gas masses
    • Multiwavelength photometry catalogs, SED fitting
    • The Environment of Galaxies
    • Interstellar dust

    Ongoing collaborations

    Publications

    Project/mission at ESA

    Hubble Space Telescope

    Website: https://www.stsci.edu/~krowlands/