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Fig. 10


Evolution of the SSFR as function of the redshift. The solid line shows the linear fit applied to the mass limited sample, while the dashed line shows the trend found by Juneau et al. (2013) for FIDEL infrared galaxies at 0.3 <z< 1.0, extrapolated to the whole interval probed. The dotted line shows the limit SSFR of our survey. The vertical lines delimit the redshift intervals used for further analysis.

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