Orbital and dynamical analysis of the system around HR 8799 - New astrometric epochs from VLT/SPHERE and LBT/LUCI

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Fig. 6

Residuals to the best-fitting, near-resonant four-planet Model 2 in Table 7 for m_⋆ = 1.47 M_⊙, a continuation of Fig. 8 for planets HR8799d and HR 8799e. See the caption of Fig. 5 for labels. The yellow star marks the GRAVITY measurement for HR 8799e.

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