Speaker
Prof.
Savvas Koushiappas
(Brown University)
Description
I will discuss the application of machine learning techniques for the detection of the astrometric signature of dark matter substructure. In this simple proof of principle example, a population of dark matter subhalos in the Milky Way act as lenses for sources of extragalactic origin. We show that machine learning applied to an SKA -like survey can be used to probe the substructure content of the Milky Way.
Author
Prof.
Savvas Koushiappas
(Brown University)