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Explore cutting-edge methods for probing astrophysics and dark sector physics through cross-correlations between Cosmic Microwave Background (CMB) and Large Scale Structure (LSS) observations in this 18-minute conference talk. Discover how multi-probe cosmological analysis techniques are advancing our understanding of fundamental physics by combining different observational datasets. Learn about innovative approaches to studying the dark sector of the universe through sophisticated statistical methods that leverage correlations between CMB measurements and galaxy surveys. Examine the latest developments in cross-correlation studies that bridge microwave background observations with large-scale structure tracers to extract new cosmological information. Understand how these combined observational strategies are opening new windows into astrophysical processes and dark matter physics that cannot be accessed through single-probe analyses alone.
