Fig. 3.

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Relative density of planets as a function of the distance to the closest MMR (left). Resonant chains and single planets are arbitrarily set at ΔMMR = 0.001 and 100, respectively. The colors indicate the method used to obtain the mass. The dark grey area indicates the 1σ confidence interval for the local mean value of ρrel, while the dotted lines show a local estimation of its scatter. Distribution of relative densities assuming gaussian distributions, binning by method and distance to the resonance (right): resonant, nearly resonant (0.001 < ΔMMR < 0.05), non resonant (0.05 < ΔMMR), and single planets.
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