Fig. 5.
Redshift histogram for the spectroscopically confirmed members and possible members (N = 31) of the protocluster around HzRG 7C 1756+6520 at z = 1.4156. The plotted redshifts come from this work, G 10, and M 12. For the protocluster galaxies in common with G 10 and M 12, we adopted our redshift determinations. Redshift bins are of 0.01 (~3000 km s−1 observed frame), corresponding to the standard deviation of the Gaussian function distribution. The vertical dashed line marks the redshift of the central HzRG 7C 1756+6520.
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