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3D weak lensing

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If you have a question about this talk, please contact Tommaso Giannantonio.

I will present a short review of weak gravitational lensing, in particular power spectrum analyses, know as cosmic shear, and how these statistics are being used now and in preparation for new facilities in particular Euclid and LSST . A full 3D power spectrum analysis of current weak lensing data will be shown, and I will discuss consistency with CMB cosmological parameter constraints.

This talk is part of the Cosmology Lunch series.

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