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Explore the future of cosmological research through cross-correlations between Cosmic Microwave Background (CMB) and Large Scale Structure (LSS) observations in this 47-minute conference talk by Simone Ferraro from Lawrence Berkeley National Laboratory. Delivered at the Kavli Institute for Theoretical Physics conference on "New Synergies in Multi-Probe Cosmology," discover how innovative methods combining multiple observational probes are advancing our understanding of astrophysics and cosmology. Learn about cutting-edge techniques in CMB-LSS cross-correlation studies, including analysis of the Sunyaev Zel'dovich effect and gravitational lensing, combined-probe analysis of galaxy clustering, measurement of the Integrated Sachs-Wolfe effect, and cross-correlations of intensity mapping with other LSS tracers. Gain insights into the synergies between gravitational wave astronomy and large-scale structure probes, while examining how ongoing and future surveys across radio, microwave, optical, and X-ray wavelengths will shape the next decade of cosmological discoveries. Understand state-of-the-art analysis techniques and get a comprehensive overview of current multi-wavelength survey capabilities that are revolutionizing our approach to studying the universe's structure and evolution.
