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Fig. 4.
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Evolution of the observed galaxy SMF of the total sample across 0.2 < z ≤ 6.5. The ℳ bins are uniform except for the first bin, which is extended to the respective stellar mass limit. The ℳ bins below the stellar mass limit (Eq. 3) are not shown. Uncertainties are indicated by the solid error bars and shaded regions.
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