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Explore weak lensing techniques without shape noise in this 33-minute lecture by Elisabeth Krause, part of the "Largest Cosmological Surveys and Big Data Science" program at the International Centre for Theoretical Sciences. Delve into advanced cosmological research methods and gain insights into analyzing large-scale structure surveys. Learn how to overcome shape noise challenges in weak lensing studies, enhancing the precision of cosmological measurements. Understand the implications for ongoing and future surveys like DES, KiDS, HSC, DESI, and LSST. Benefit from expert knowledge in multi-messenger cosmology and develop skills to utilize publicly available data for cutting-edge research in the field.
