Fig. 9

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[C/H] for the HKB-fid simulation as a function of time. The filled areas correspond to predictions for Uranus (purple) and Neptune (blue). The uncertainties are shown via the extension of the filled areas and are due to uncertainties on the respective atmospheric masses. The solid and dashed black lines are the maximum estimation of the gas disc contribution obtained from observations for Uranus and Neptune (see Section 3.1.1).
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