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Fig. 12


Stability indicator (defined in Eq. (3)) for TOI-178 as a function of the periods and eccentricity of planet f (top). The red areas show the initial conditions of unstable trajectories, while black shows stable (quasi-periodic) trajectories. Bottom panel: same stability criterion with respect to the initial periods of planets f and g. The dashed white lines show the observed periods reported in Table 4.

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