My research focuses on the search for indirect signals from dark matter annihilation in the universe. I am also interested in the usage of neutron stars as probes for new physics, the astrophysics of the Galactic Center region, and the evolution of massive binary stars.

Together with a number of colleagues, my most recent work centers on the identification and modeling of a new class of TeV sources, named "TeV halos". I am currently working to understand these emission sources, and make predictions for upcoming observations by HAWC, HESS, and CTA.