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

• SPOGs - K. Alatalo (STScI, USA), K. D. French (UIUC, USA), L. Lanz (TCNJ, USA), http://www.spogs.org/
• SDSS MaNGA, https://www.sdss.org/
• UKIDSS Ultra-Deep Survey - O. Almaini (University of Nottingham, UK), V. Wild (University of St Andrews, UK), https://www.nottingham.ac.uk/astronomy/UDS/

Publications

• ADS
• ORCID: https://orcid.org/0000-0001-7883-8434

Project/mission at ESA

Hubble Space Telescope

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