Institute for Advanced Study/Princeton University Early Universe/Cosmology Lunch Discussion

With upcoming arcminute resolution multi-frequency CMB maps and full-sky galaxy surveys, observables based on the Sunyaev Zeldovich (SZ) effect will constitute a promising avenue for reshaping our understanding of galaxy formation and constraining cosmological models. We will start by briefly reviewing current measurements of the thermal and kinetic SZ effects, before presenting theoretical modeling, measurements and constraints involving a new set of observables based on a three-point statistics between the kinetic SZ effect and large scale structure (LSS) tracers: projected fields kSZ$^2$-LSS power spectra.