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Fig. 4

image

Best-fit parameters of the NFW mass model for the stacks in richness N (red triangles), luminosity L (orange disks), SIS velocity dispersion σv (blue squares), and arc radius RA (purple stars). The large black rectangle shows the M200⟩ ± 1σ and c200⟩ ± 1σ obtained using the 80 groups (stack S0). The green-hatched area delimits the 1σ uncertainty around the mass-concentration relation derived with Lenstool, using a M200(σv) scaling.

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