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Fig. 2.

image

Observed velocity dispersion (σv, obs) of groups determined using their spec-z members within r200c versus the velocity dispersion predicted by the virial theorem (Eq. (3), σv, VT), in COSMOS based on Lx- halo mass scaling relation in observations (upper panel) and using the virial mass in the HORIZON-AGN simulation (lower panel). Groups with N ≥ 5 are plotted with filled blue circles and red squares. Groups with N ≥ 10 spectroscopic members are shown with open green circles. The solid and dashed black lines show the 1:1 relation and ±15% intervals. The filled red squares and blue circles represent groups in S-I and S-II to S-IV respectively.

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