Fig. 5

Right: edge-on coplanar grid with jitter included. The
eccentricities of both planets are varied in the range from 0.001 to 0.251 with
steps of 0.005, while the other orbital parameters and the zero-point offset were
fitted until the
minimum is achieved. The solid black
contours indicate the stable fits, while the dashed contours indicate fits where the
system survives the dynamical tests, but with chaotic scattering behavior. While the
best dynamical fit is unstable (white star), we found two stability islands where
long-term (108 yr) stability is achieved. With a moderate
eb, at the
1σ
border (blue contours), a stable 2:1 MMR region exists, and at lower eccentricities
a broad stability region can be seen at more than 3σ from the best fit,
without showing any signs of a low-order MMR. Left: higher
resolution zoom of the stable 2:1 resonant region.
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