I am an astrophysicist and science communicator.

At DAWN, my tasks include communicating our science to the public, arranging workshops, coordinating other scientific activities, maintaining our website, as well as conducting my own research.

My research focuses on galaxies, in particular the light coming from processes that have to do with galaxy formation. I use computer simulations to predict and interpret "real" observations. More specifically, I use hydrodynamical simulations with (Monte Carlo) Lyman α radiative transfer.

After my PhD I was a postdoc at the Oskar Klein Centre (U. of Stockholm), the Dark Cosmology Centre (UCPH), and the Cosmology and extragalactic astronomy section (U. of Oslo).

You can find out more about me, my research, and my outreach activities on my personal website.