Staff profile

• Star formation
• High-redshift galaxies
• Gas dynamics
• Molecular and ionised gas

Journal Article

• The properties of the interstellar medium in dusty star-forming galaxies at z ∼ 2–4: the shape of the CO spectral line energy distributions
  
  Taylor, D. J., Swinbank, A. M., Smail, I., Puglisi, A., Birkin, J. E., Dudzevičiūtė, U., Chen, C.-C., Ikarashi, S., Frias Castillo, M., Weiß, A., Li, Z., Chapman, S. C., Jansen, J., Jiménez-Andrade, E. F., Morabito, L. K., Murphy, E. J., Rybak, M., & van der Werf, P. P. (2025). The properties of the interstellar medium in dusty star-forming galaxies at z ∼ 2–4: the shape of the CO spectral line energy distributions. Monthly Notices of the Royal Astronomical Society, 536(2), 1149-1165. https://doi.org/10.1093/mnras/stae2642
• An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies
  
  Liao, C.-L., Chen, C.-C., Wang, W.-H., Smail, I., Ao, Y., Chapman, S. C., Dudzevičiūtė, U., Frias Castillo, M., Lee, M. M., Serjeant, S., Swinbank, A. M., Taylor, D. J., Umehata, H., & Zhao, Y. (2024). An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies. The Astrophysical Journal, 961(2), Article 226. https://doi.org/10.3847/1538-4357/ad148c