Extended Data Table 4 Distance of the estimated generalized three-body Laplace angle Ψe=0 to the closest equilibrium for all period ratios that are not excluded by available observations

From: A resonant sextuplet of sub-Neptunes transiting the bright star HD 110067

  1. Case A assumes that the mono transit at 2641.5778 TJD belongs to the fifth planet and that at 2656.0944 TJD belongs to the sixth planet. Case B assumes the opposite. The flag column * = 1 indicates that the position of the equilibria varies with the masses of the planets, in which case the equilibrium is recomputed using ref. 164, with masses computed using a mass–radius relation for sub-Neptunes26. For * = 0, the equilibrium is 180°.
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