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Fig. 1

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Star formation rate (top panel) and stellar mass distribution (bottom panel) as function of redshift for the 24  μm-selected star-forming population. The horizontal gray lines in the top panel indicate the SFR thresholds corresponding to luminous and ultra-luminous infrared galaxies (i.e., LIRGs and ULIRGs). The solid red line in the bottom panel indicates the 50% completeness limit (i.e., M50%(z), see Sect. 2.2.2).

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