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Fig. 6
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Posterior distributions of the sampled scaled planetary radii Rb/R★ for the TESS and MuSCAT2 g′, r′, i′, zs bands. The solid and dotted, vertical, gray lines mark the median and the 68.3% credibility interval of the Rp/R★’s posterior distribution, as derived in case 2 (see Sect. 4.1).
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