Fig. 6.

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Projected two-point correlation functions corresponding to different redshift bins (as labelled) in the magnitude ranges −24 < MW1 ≤ −23 (left panel) and MW1 ≤ −24 (right panel). The insets show the best fitting power-law parameters with 1σ error contour. The error bars on the markers are the square root of the diagonals of the covariance matrix obtained from the jackknife resampling method.
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