Impact of the local Universe SZ signal on the lack of correlation at angular scales θ > 60°. We measure the difference of S​_1/2 (see Eq. (4)) between Gaussian CMB realizations with or without the local tSZ (at 143 GHz) and kSZ effects, when the galactic plane alone was masked (in red), and when the galactic plane and Virgo were masked (in green). The distributions are shown for both the full set (solid lines) and for the 5% (dashed) simulations where the lack of correlation is strongest (smallest S​_1/2).