Angular auto-correlation function of the selected LBG candidates around W0410–0913 (red stars), W0831+0140 (grey solid circles), and W2246–0526 (blue squares). We used logarithmic binning of the separations to ensure sufficient pair counts at small separations. The lines represent the power-law fits (red dotted lines): for W0410–0913 and W0831+0140, the separation angle ranges from 3 arcseconds to 480 arcseconds, with power-law fits (grey solid lines) of A_ω = 13.07 ± 3.31 and β = 1.244 ± 0.08; and A_ω = 5.28 ± 2.51 and β = 1.30 ± 0.16, respectively. For W2246–0526, the separation angle ranges from 2 arcseconds to 480 arcseconds, with power-law fits (blue dashed lines) of A_ω = 3.82 ± 3.19 and β = 0.99 ± 0.24.