Left panel: Distribution of our z ∼ 1 MIRI-selected SFGs over the SFR–M_⊙ correlation at z ∼ 1. The SFR and M_star are obtained from the SED analysis. The green dashed line is z = 0.8 − 1.2 MS relation of Elbaz et al. 2007. The orange dashed line is z = 1.1 − 1.4 the MS relation from Pearson et al. 2018. The gray diamonds are the MIRI-selected SFGs sample of Lin et al. 2024. The majority of our z ∼ 1 sample is consistent with the MS relation of Elbaz et al. 2007. Right panel: Distribution of our MIRI-selected SFGs at z ∼ 2 over the SFR–M_⊙ correlation at z ∼ 1. The distribution of the z ∼ 2 SFGs indicates an evolution compared to z ∼ 1 MS.