Sebastian Kiehlmann received his diploma in Physics at the University Göttingen (Germany) in 2010 and his PhD in Experimental Physics at the University of Cologne (Germany) for a thesis written at the Max Planck Insitute of Radio Astronomy in Bonn (Germany) in 2015.
He was a postdoctoral researcher at the Metsähovi Radio Observatory of the Aalto University, Espoo in Finland in 2015/2016. From 2017-2019 he was a staff researcher at the Owens Valley Radio Observatory and California Institute of Technology in the USA. He joined the Institute of Astrophysics in Crete in spring 2019 as postdoctoral researcher.
Active galactic nuclei; blazars; astronomical jets; radio astronomy; high-energy astrophysics; optical polarization; time domain astronomy.