Orbital solutions for stars at the GC found in Gillessen et al. (2017), with the exception of S5, which is from von Fellenberg et al. (2022). Stars that are considered part of the young disc are coloured blue, which are S66, S67, S83, S87, S91, S96, S97, and R44. S111 is omitted, because of the hyperbolic solution. The grey points show S-stars fainter than our completeness limit, while black points show those that are brighter.