Same as Fig. 4 but for data simulated with the XRISM Resolve micro-calorimeter. The exposure time was assumed to be 200 kiloseconds. The physical sizes of inner shells are approximately (0–3) kiloparsecs for NGC 4636, (0–16) kiloparsecs for Perseus and A262, (0–54) kiloparsecs for A1795, (0–66) kiloparsecs for A2029, and (0–142) kiloparsecs for A383. The physical sizes of outer shells are approximately (3–7) kiloparsecs for NGC 4636, (16–33) kiloparsecs for Perseus and A262, (54–108) kiloparsecs for A1795, (66–133) kiloparsecs for A2029, and (142–283) kiloparsecs for A383. The errors represent the standard deviation 1σ. Similar to Fig. 4, the best-fit values of the 2T model, for which the second CIE component was not significant, were removed from this plot (see the last paragraph of Sect. 2.4). The 1T model results of A383 for the best-fit temperature in both radial bins are plotted with an empty diamond point for visualisation purposes.