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Separating the Weak Lensing and Kinetic Sunyaev‐Zeldovich Effects from Cosmic Microwave Background Temperature Maps
A new generation of CMB experiments will soon make sensitive high resolution maps of the microwave sky. At angular scales less than $\sim$10 arcminutes, most CMB anisotropies are generated at z $< 1000$, rather than at the surface of last scattering. Therefore, these maps potentially contain an enormous amount of …