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Fig. 2


Star formation rate from the SED fitting as a function of stellar mass for all the galaxies in our sample. The curves represent the main sequence of galaxies derived by Tomczak et al. (2016) for the redshifts of 1.5, 2.5, and 3.5. The color corresponds to the value of Δ SFR = log(SFR∕SFRMS), the offset from the main sequence. The typical error bar for individual points is shown in the lower right corner.

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