Fig. A.7
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Corner plot for the H2/He scenario of GJ 3090 b showing the posterior distributions for the planet mass (M), radius (R), atmospheric mass fraction (AMF), core mass fraction (CMF), and refractory element ratios (Fe/Mg and Fe/Si). The red contours correspond to the case with stellar-informed priors on the refractory abundances, while the black contours correspond to the case without such priors. The inclusion of stellar priors significantly reduces the spread in CMF and AMF values by constraining the rocky interior composition.
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