Figure 8.
Distribution of rest-frame (NUV−r) for the final passive (NUV + WISE red sequence) sample versus the multiplicity of the group containing the galaxy (top panel), and versus group velocity dispersion σ (bottom panel). The bottom panel can be compared to the upper right panel of fig. 4 in Ali et al. (2019).

Distribution of rest-frame (NUV−r) for the final passive (NUV + WISE red sequence) sample versus the multiplicity of the group containing the galaxy (top panel), and versus group velocity dispersion σ (bottom panel). The bottom panel can be compared to the upper right panel of fig. 4 in Ali et al. (2019).

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