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Fig. 1


Cumulative SFR distributions of our sample (solid black line) and its z> 0.5 subsample (solid blue line). Shaded regions show the 1σ sampling range around solid lines. Dashed lines show distributions including lower limits. For comparison we also plot a star-formation-weighted distribution of z = 0.8 star-forming galaxies (Ly et al. 2011) (red solid line), the same distribution extrapolated towards lower SFRs to account for the completeness limit of the survey (red dotted line), and the z> 0.3 VVDS sample (light blue line; see text for details).

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