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., 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., Chen, C., Wang, W., 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