Fig. C.1
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Comparison of NAMD values for the Kepler-462 system. The system consists of two planets on eccentric and misaligned orbits. Top: R-NAMD as defined in T20 using relative inclinations. Middle: λ-NAMD, using the projected spin–orbit angle (λ). Bottom: A-NAMD as defined in this work using the spin–orbit angle (ψ). The A-NAMD metric is the most suitable to capture the true architecture of the system.
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