Fig. 1

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Schematic view of Jupiter’s interior model used in this study (left) and the exploration workflow (right). The model’s free parameters are shown. For each step of the exploration, we state which method is being used, which observables are used to constrain the solutions, and the number of plausible models resulting from this step. The prediction errors of NeuralCMS are denoted by ϵ (Ziv et al. 2024).
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