Fig. D.1
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Corner plots from the interior modeling of TOI-756 b (see Sect.6.2.2). The top panel shows scenario (1), assuming a H/He envelope: results with uninformative priors are shown in grey, and those using stellar-informed priors based on the host star’s refractory abundances are in red. The bottom panel corresponds to scenario (2), assuming a pure H2O envelope with stellar-informed priors.
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