Fig. 4.
Histogram of the velocity offset between Mg ii-based redshift and [C ii]-based redshift ($\Delta v = v_{\rm Mg\, \small {II}} - v_{\rm [C\, \small {II}]}$) for $z \gt 5.7$ quasars compiled from the literature (Maiolino et al. 2005; Venemans et al. 2012, 2016, 2017c; Wang et al. 2013, 2016; Willott et al. 2013, 2015, 2017; Bañados et al. 2015; Mazzucchelli et al. 2017; Decarli et al. 2018), along with our HSC quasars. The Mg ii line is predominantly blueshifted in these $z \gtrsim 6$ quasars with a mean and standard deviation of $-284 \pm 607$ km s$^{-1}$. (Color online)

Histogram of the velocity offset between Mg ii-based redshift and [C ii]-based redshift (⁠|$\Delta v = v_{\rm Mg\, \small {II}} - v_{\rm [C\, \small {II}]}$|⁠) for |$z \gt 5.7$| quasars compiled from the literature (Maiolino et al. 2005; Venemans et al. 2012, 2016, 2017c; Wang et al. 2013, 2016; Willott et al. 2013, 2015, 2017; Bañados et al. 2015; Mazzucchelli et al. 2017; Decarli et al. 2018), along with our HSC quasars. The Mg ii line is predominantly blueshifted in these |$z \gtrsim 6$| quasars with a mean and standard deviation of |$-284 \pm 607$| km s|$^{-1}$|⁠. (Color online)

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