Fig. 1.
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Projection of galaxy distributions of samples σ0, σ5, σ10 in a slice with a thickness of 10 Mpc. Each dot represents a galaxy. The photometric uncertainties are parallel to the z-axis, which also defines the line of sight in this work. Only an area of 150 Mpc × 150 Mpc is shown for visual clarity. For information about samples; see Sect. 2.3.
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