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Fig. 4.

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2D histograms of for each possible pair of the weight number count ratios considered in this work. The weights we were computed with a 45″ aperture and limiting magnitude i < 24. The jagged histogram for the unweighted counts is due to the relatively small number of galaxies in an aperture of this size. The inner and outer contours represent 68 and 95% confidence intervals, respectively.

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