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This talk focuses on evolution of galaxies similar to the Milky Way. Magnification from gravitational lensing offers a promising way to study these galaxies at intermediate redshifts, which are otherwise poorly resolved in current surveys. I discuss measurements of gas kinematics and chemical abundances, which reveal in situ formation of thick disks in Milky Way-like galaxies at z~2.
Discs in galaxies
Discs in galaxies
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