Fig. 12

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Global stability analysis of the WASP-148 planetary system. We fixed all orbital parameters of the stable MAP solution (Table 4), and we varied the inclination, ic, and the longitude of the ascending node, Ωc, of planet-c. The step size is 0.25° in both axes. For each initial condition, the system was integrated over 50 kyr and a stability criterion was derived with the frequency analysis of the mean longitude. White dashed curves give the isolines of constant mutual inclination I = 10°, 20°, 30°, and 40°. The white dot marks the position of the stable MAP solution from Table 4. The colour bar corresponds to the one in Fig. 11.
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