Similar to Fig. 5, but using a reconstructed SZ map that now uses all six HFI frequency channels. The noise in all maps is reduced by the inclusion of the two highest frequencies. Stacked images in the stellar-mass bins above log ₁₀(M_∗/M_⊙) = 11.25 are not significantly affected, but for the low stellar-mass panels, the extended signal near map centre is larger and has higher signal to noise than in Fig. 5, suggesting that it may be real SZ signal broadened by miscentering effects.