Posterior distributions of the planetary radii derived from the analysis of the available light curves, which include our version of the TESS light curve, which was detrended using two different algorithms, as described in Sect. 2.1. We also show the posterior distributions corresponding to the radius measurements available in the literature. The posteriors for planet b corresponding to the measurements of Osborn et al. (2022) and Zhang et al. (2023) are equal and, therefore, they are not discernible.