Pressure profiles (top panel) and intrinsic scatters (bottom panel) for our sample and literature works, with literature errors omitted from the top panel for clarity. Within r₅₀₀, our profile is ∼12% lower than the UPP, close to what is needed to remove the tension in cosmological parameters derived from CMB and Planck SZ cluster counts (Ruppin et al. 2019). The steep decline of our pressure profile beyond r₅₀₀ is consistent with the deficit reported by Anbajagane et al. (2022), interpreted as a shock-induced thermal nonequilibrium between electrons and ions. Regarding the scatter, the three radial profiles are consistent up to 0.4r₅₀₀. Beyond this radius, Sayers et al. (2023) report the highest scatter, while our analysis yields the lowest.