Stellar mass distributions (top panel) and SFR distributions (bottom panel) as a function of redshift for the 24 μm sample. The solid blue line represents the 50% mass completeness limit of the FIR sample (see text), while the orange line represents the stellar mass completeness of the HSC-CLAUDS K-selected sample (K ≤ 24.5; see text). The horizontal gray lines in the bottom panel indicate the SFR threshold that corresponds to the luminous (LIRG, L_IR ≥ 10¹¹ L_⊙) and ultra-luminous (ULIRG, L_IR ≥ 10¹² L_⊙) infrared galaxies.