Coloured dots gives the stellar density derived from MCMC analyses of transits from a single planet, solid black line gives the density derived from a global analysis of all transits observed with its 1-σ uncertainty in gray shades. Colorbar shows the number of transits used in each analysis. Solid blue line give the stellar density value computed by Agol et al. (2020) using a photodynamical model created with the mass-ratios and orbital parameters derived from a transit-timing analysis, with its 1-σ uncertainty in blue shades.