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Fig. 6.

image

Dressler-Shectman (DS) plot. It shows the x, y location of the spectroscopically-confirmed proto-cluster members, centered on 7C 1756+6520. The DS test is applied to proto-cluster members with z within the range [−3σcl, +3σcl] from zcl. The radii of the plotted circles are proportional to eδ/2, where δ is the DS measurement of local deviation from the global velocity dispersion and mean recession velocity (cf. Eq. (2)). Depending on in which bin falls, the circles are: blue and dashed [−3σcl, −1σcl], green [−1σcl, +1σcl], red and hashed [+1σcl, +3σcl]. The black and dotted circle is the galaxy MSC2, excluded from the DS test because it has a that does not fall in the range [−3σcl, +3σcl]. The number of proto-cluster members Ng, the statistics Δ, and the statistical significance P are also given on the figure.

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