Fig. 6

SED-derived star formation rate as a function of stellar mass. The MASSIV sample (Wide = green circles, Deep = red squares and Ultra-Deep = blue triangles) is compared to the VVDS parent sample (small filled squares). The lines represent the empirical relations between SFR and stellar mass for different redshifts between z = 0 and z = 3 following the analytical expression given in Bouché et al. (2010).
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