Marko Stalevski, PhD

Astrophysicist studying dust and gas  swirling around supermassive black holes, know as Active Galactic Nuclei (AGN). PhD degree from a joint program by University of Belgrade, Serbia and Ghent University, Belgium. Main line of work involves modeling and interpreting the emission coming from the dusty clouds in these objects. Part of the team developing state-of-the-art Monte Carlo radiative transfer code called SKIRT. Also interested in the phenomena of graviatational lensing and AGN variability.