Gas content of the satellite galaxies in relaxed (left panels) and disturbed clusters (right panels), for low- (upper panels), and high-redshift (bottom panels). In those panels, in contrast to Figure 11, we exclude the second BCG in the case of disturbed halos. Each panel shows the gas content for each gas phase: hot, diffuse, and condensed. We can see that the hot gas content decreases, but we can see that on average galaxies in disturbed clusters contain more diffuse and condensed gas.