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


  • 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


Project/mission at ESA

Hubble Space Telescope

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