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Fig. 9.
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Probability density distributions of MUV, the UV slope, the EW(Lyα), the SFR, the ΣSFR, and sSFR from top left to bottom right for objects with 
> 25.2 (filled blue histogram) and objects with 
< 25.2 (empty black histogram). Only galaxies with log(Mstar/M⊙) > 9.5 are considered in both cases.
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