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I will present results from Hubble and Keck surveys of lensed galaxies behind massive lensing clusters. The first data reveal a large number of dwarf galaxies at z~2 a factor of 100 fainter than previous studies, with no sign of a turnover in the luminosity function. I will show why these dwarf galaxies likely behave differently from their more massive counterparts, and will preview preliminary results on their dust extinction and escape fraction of ionizing photons.
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