Fig. 8.
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Observed UV slope measured by fitting a power law spectrum to the F115W and F150W photometry. The shown MUV is computed from the best-fit used to obtain βUV. COLA1 presents a steep slope in comparison with other bright [O III] emitters in C1F. Only objects with S/N > 5 in F115W and F150W are shown. We also compare with the estimated average βUV in Bouwens et al. (2014) for LBGs at z ∼ 6.
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