Fig. 1.
Redshift distribution of our galaxies plotted against their (dust-corrected) SFR (1σ error bars are in grey). The colour denotes the stellar mass. The solid line depicts the lowest uncorrected SFR from Hβ λ4861 we can detect in the HUDF at each redshift (which is effectively determined by the requirement that S/N(Hγ λ4340)> 3; see Sect. 2.4).
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