Fig. 11
Planetary radii derived in this study (dashed lines) in comparison with those reported by Batalha et al. (2013, BA13), Huber et al. (2013, H13), Rowe et al. (2014, R14), Rowe et al. (2015, R15), Johnson et al. (2017, J17), Fulton & Petigura (2018, FP18), Berger et al. (2018, BE18) indicated by red and green filled circles for Kepler-278b/c (left) and Kepler-391b/c (right), respectively. Grey shaded areas indicate 1σ uncertainty in our results.
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