Fig. 3.

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Top: Radial correlation matrix for the Wiener filtered field. Bottom: Radial correlation matrix for the unfiltered field. For both fields the galaxy density is Ngal = 20 per square arcminute. Note: the correlation matrices are limited between 0 and 1 (instead of between −1 and 1) to see the difference between the two correlation matrices more clearly. Here, the radial bins are linearly spaced bins between 0 and 10 arcminutes.
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