Comparison of σ_Tj, int/T estimated in cells of 0.1R₅₀₀ as a function of radius between the CHEX-MATE objects (blue; the 16th and 84th percentiles were computed excluding the annuli for which the statistical errors prevents a proper determination of the intrinsic scatter) and results extracted from various hydrodynamical simulations (see text for details in Sect. 4.1). For cosmological simulations (i.e., The 300 GX and GIZMO), we represent the distribution for 45 objects with the median and a dispersion equal to the inter-quartile range divided by 1.35. For the FLASH simulations, we present the results obtained for 3 different projections (with different line styles) of the same object simulated with two different levels of turbulence (i.e., different Mach).