Notes. ⁽¹⁾The orbital period and mutual inclinations are not direct results of the orbit fit, but are calculated from the posterior distribution. ⁽²⁾In absence of any radial velocity data, there is a degeneracy in Ω and ω, and a second, equally valid, solution can be obtained by adding 180 deg to both ω and Ω. This also results in a degeneracy in the mutual inclinations, with θ_out = 68.45 ± 1.54 deg or 50.5−58.5 deg being a second set of valid solutions. ⁽³⁾Using the parameters reported in Bohn et al. (2022) for the outer disc. ⁽⁴⁾Using a range of 20–28 deg for the inclination of the outer disc, and Ω_out = 160 deg (Verhoeff et al. 2011; Perez et al. 2014; Boehler et al. 2017; Price et al. 2018a; Garg et al. 2021).