Fig. 7
Angular correlation function for the sample of 21 LBG candidates at z ~ 6 (red) and for the sample of 22 contaminants (green, slightly shifted for clarity) of Table 3. A positive (~3σ) signal is measured at θ< 10 arcmin for highz galaxies, whereas a null correlation is observed for the contaminants. The red dashed line is the best fit to the highz galaxy correlation function including the integral constraint.
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