Mass-radius diagram for heavy planets, brown dwarfs and low-mass stars. The radius axis corresponds to the size range of Jupiter-mass planets discovered so far. Inverted blue triangles show eclipsing/transiting SB1s, upright red triangles denote interferometric measurements. The two (M₂, R₂) posterior probability density distributions for WASP-30b and J1219–39b are drawn in grey with their 1 − σ confidence regions in white. Models by Baraffe et al. (2003, 1998) are also displayed with ages 5 Gyr (black), 1 Gyr (dark grey), 500 Myr (light grey) and 10 Gyr (dotted). Models are for [M/H]  = 0. Observational data were taken from Lane et al. (2001); Ségransan et al. (2003); Pont et al. (2005a,b, 2006); Beatty et al. (2007); Deleuil et al. (2008); Demory et al. (2009); Bouchy et al. (2011); Johnson et al. (2011); Ofir et al. (2012); Siverd et al. (2012).