Stars from our ED-2 samples in R − z space, with velocities indicated as trails. In blue are the true known members from our 6D Gaia RVS sample. In orange, the likely members of ED-2 inferred from 5D information, without known v_los, by our method. The velocities are predicted from the most likely v_los corresponding to the peak of the PDF. In red, the stars were inferred without using the additional phase information of ED-2 (described in Sect. 4.2). Both of these samples have been selected with a minimum probability of p_min = 50%, corresponding to an expected purity of 86% with phase information and 56% when assuming the structure is phase-mixed.