Fig. 3
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Same as Fig. 1, but for a system that became unstable after the gas–disc phase with no surviving inner planets. We mark all surviving planets in colour. The planet marked in orange acquires some eccentricity during the gas–disc phase, preventing pebble accretion, and it only continues to grow once its eccentricity is damped below 1%. The system corresponds to system number 1 in Fig. C.1.
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