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Fig. A.1

image

Angular completeness as a functionof the pair separation angle θ estimated using the VIPERS mocks. All measurements are performed over the redshift range 0.6 ≤ z ≤ 1.0. The auto-correlation statistic of the full magnitude-limited sample (red continuous line) provides estimates of wA almost identical to those obtained using auto-correlation of volume-limited samples of blue galaxies (blue dots) and their cross correlation (green crosses) with the red ones.

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