Fig. 8.

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Probability distributions for rv (first column), (second column), and λv (third column) for voids identified in the calibrated Buzzard mocks (purple) and in the Legacy Survey (orange). The void samples are subdivided into four equispaced redshift bins with Δz = 0.15, with the redshift increasing for each row from top to bottom. The excellent agreement between the properties of the observed and simulated voids ensures effective control of systematics related to potential mismatches between observations and simulations.
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