Average H I mass (top panel) and average H I-to-stellar mass ratio (bottom panel) in different radial and mass bins for galaxies in relaxed clusters (open squares) and disturbed clusters (open diamonds), compared with the full cluster sample (open circles). For clarity, data points at the same radial bin are horizontally offset by 0.1 dex to avoid overlapping error bars; the offset has no physical meaning. While the overall trends are consistent with those of the full cluster sample, the total stacked signal may fall outside the relaxed and disturbed values due to baseline subtraction and the exclusion of five galaxy clusters from the stack, although the associated uncertainties remain self-consistent. A roughly 1σ difference is observed in the innermost radial bin, potentially indicating a mild dependence of the gas content on the cluster dynamical state. The splashback radius of clusters at ∼1.5, R₂₀₀ is shown by the vertical dashed line (T. Shin et al. 2019).