Fig. C.2.
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Marginalised posterior distributions of three parameters obtained using an MCMC method for the halo model to fit ΔΣ(P(z > zl + 0.2) > 0.98) around the galaxies of the FLS. The three contour levels, from outermost to innermost, correspond to 16%, 50%, 84% confidence levels, respectively. The blue points and lines are the medians.
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