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Fig. 5.
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Galaxy UV luminosity functions at z = 10, as in Fig. 3. Data points from B20; Bouwens et al. (2019), Morishita et al. (2018), Oesch et al. (2018) are shown. The best-fitting double power-law function from B20 and the Schechter function from Oesch et al. (2018) are displayed.
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