Fig. 5.
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Observed total galaxy SMF of DAWN PL (coloured points) and uncertainties (1σ, shaded) compared with two measurements from COSMOS, D17 and W23, through to 3 < z ≤ 3.5. ℳ bins below the stellar mass limit (Eq. 3) are not shown. The volume limit according to the N = 0 Poisson uncertainty is shown by the downward pointing coloured arrow for DAWN PL and in grey for W23.
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