Georgios Magdis

Georgios Magdis is an Associate Professor in the Department of Space Research and Technology at the Technical University of Denmark (DTU), specializing in Astrophysics and Atmospheric Physics. He also holds an external position as Affiliated Associate Professor at the University of Copenhagen since 2021. His research focuses on galaxy formation and evolution across cosmic time, with particular expertise in high-redshift galaxies, star formation processes, and the interstellar medium.

Magdis's research interests center on galaxies and their evolution, with specific focus areas including star formation (93% of his work), stellar mass (79%), star formation rates (65%), spectral energy distribution (45%), molecular gas (39%), interstellar matter (38%), and active galactic nuclei (36%). His work heavily utilizes cutting-edge observational facilities including JWST, ALMA, and NOEMA, with research spanning from the local universe to the cosmic dawn. He has published 116 research outputs, with a significant portion focusing on early universe galaxy formation and evolution.

His recent publications reveal a strong emphasis on high-redshift galaxy studies using JWST data, with particular interest in galaxy structure, star formation processes, and dust properties in the early universe. His work often involves large international collaborations, particularly with the COSMOS-Web survey, which represents one of the most ambitious JWST projects to date. His research frequently combines multi-wavelength observations to build comprehensive models of galaxy evolution across cosmic time.

Magdis actively supervises multiple PhD students and leads significant research projects including 'The Hidden Cosmos' and 'Unveiling the physics of galaxies and structure assembly in the early Universe.' His work has generated several important datasets, including the NOEMA formIng Cluster survEy (NICE), which has been widely referenced in the astronomical community.