Open Access

Fig. 7.

image

Cross-correlation function as a function of r for two lowest values r = [2, 6] h−1 Mpc. The red curves indicate the best-fit model of the standard fit obtained for the fitting range 10 <  r <  180 h−1 Mpc. The curves have been extrapolated outside this range. The imprints of quasar–metal correlations are visible as peaks indicated by the dashed black lines at r ≈ −21 h−1 Mpc (SiIII(120.7)), r ≈ −53 h−1 Mpc (SiII(119.0)), r ≈ −59 h−1 Mpc (SiII(119.3)), and r ≈ +103 h−1 Mpc (SiII(126.0)).

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