Evolution of the fraction of quenched satellite galaxies (top and circle markers) across cosmic time compared with the quenched fraction of field galaxies (bottom and square markers) for each model. Markers indicate the mean f_q for each time bin, and the error bars represent the standard deviation. In the row where we show the quenched fraction of the satellites, we also display that of the field galaxies with higher transparency and vice versa to facilitate comparison. We follow the quenching definition described in Section 2.3. The orange and red shaded regions represent the epochs when the host halo is more massive than 5×10¹¹ M_⊙ and 10¹² M_⊙, respectively. The time domain where snapshots are still not available for each specific code are indicated as a gray shaded region. Quenched fractions for satellite galaxies and field galaxies above and below M_peak = 10¹⁰ M_⊙ are shown in different colors.