Fig. 11.

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Stacked images of the simulated cross-correlation from the Buzzard mocks (top) and the observed (bottom) cross-correlation between the full-sky void data set from the Legacy Survey and the Planck CMB convergence map. The first column displays the stacked images for the full void population, while the subsequent three columns correspond to void bins categorized by λv, ranging from positive to negative values. Despite the presence of instrumental noise in the observed stacked CMB patches, the images exhibit strong visual agreement between simulations and observations, clearly illustrating the distinct properties of the different void populations analyzed.
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