My research lies at the interface of cosmology and galaxy evolution. I use
multi-wavelength observations of the cosmic microwave background (CMB), the cosmic
infrared background (CIB), line intensity mapping (LIM), and large-scale structure
(LSS) tracers to probe both the fundamental physics of the universe and the star
formation history of galaxies. I also develop novel theoretical tools and
cross-correlation techniques for current and upcoming cosmological surveys.