Fig. 8
Shapes of the orbits for each of the exterior perturber TTV solutions. The dashed lines represent the orbits for the transiting planet in each case. The axis units are in terms of the semi-major axis of the transiting planet. The exact values for the mass and period ratios are specified in Table 4. The solution just interior to 3:2 is not plotted due to high χ2 values.
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