Left: M-R diagram comparing obtained M-R relations when using different EOS for water: the polytropic EOS of Seager et al. (2007) (brown), QEOS assuming temperatures of 300 and 1200 K (More et al. 1988), and ANEOS (Thompson 1990) with a surface temperature of 500 K. Right: M-R diagram comparing obtained M-R relations when using different cuts for the mass and radius uncertainties when building the revisited catalogue: σ_M ∕M = 25% and σ_R ∕R = 8%, and σ_M ∕M = 50% and σ_R ∕R = 16%. The grey envelope corresponds to the difference between the two. Blue circles represent the exoplanets with σ_M ∕M = 25% and σ_R ∕R = 8%, and red triangles represent the planets with uncertainties between σ_M∕M = 25% and σ_R ∕R = 8%, and σ_M ∕M = 50% and σ_R ∕R = 16%.