Extended Data Fig. 6: Gas mass fraction of the HD 110067 planets as a function of their equilibrium temperature.
From: A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067
We infer two values per planet by assuming the different planetary masses from our method I (red) and method II (blue) radial velocity analyses. The boxes, orange lines, green triangles and red stars represent, respectively, the 25th and 75th percentiles, medians, means and modes of the posterior distributions. The opacity of the vertical lines is proportional to the posterior distribution.
