Dependence of the derived physical quantities on the initial rotation rates, showing UV slope (β), dust attenuation in the V band (A_V), dust index (n), half-mass time (the lookback time at which 50% of the stellar mass formed), stellar mass, and specific star formation rate. The mock galaxies are generated with an SPS model of a non-rotating model (ω_i = 0.0), and the physical quantities of these mock galaxies are then estimated with models of different rotation rates (ω_i = 0.0, 0.3, 0.6, and 0.9). For each quantity, the results are grouped into three redshifts from z = 9.0 to 11.0. The colored curves represent the results binned by log(M/M_⊙), with legends shown in the top-right subplot. A minor shift is applied to ω_i for better visualization.