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Fig. 9

image

Evolution of the SFR as function of the redshift. The points show the SFR values derived either from [OII], Hβ, or Hα lines in the mass limited sample. The solid line shows the linear fit applied to the sample, while the dashed line shows the trend found by Silverman et al. (2009) for zCOSMOS star-forming galaxies at 0.48 <z< 1.05, extrapolated to the whole interval probed. The dotted line shows the limit SFR estimated for our survey, taking dust reddening and Balmer absorption corrections in account. The vertical lines delimit the redshift intervals used for further analysis.

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