New analysis methods for mapping the small-scale distribution of dark matter with strong gravitational lensing
Yeshar Hezveh
Stanford University

In yesterday's talk, I discussed how new lenses, new telescopes, and new analysis methods are about to transform the field of strong lensing in general and in particular to allow us to measure the distribution of dark matter on small scales with high precision. Today I will delve a bit deeper into these topics. I will talk about the development of new methods that can allow us to increase our sensitivity to subhalos and discuss specific projects for the next few years.