Properties of candidate ejected stars. Top: galactic coordinates of the λ Ori cluster members (black) with members that traceback to within the core radius (CA < r_c) in red, members that traceback to the core radius within 1σ (CA − σ < r_c) in yellow, members that traceback to the core radius within 2σ (CA − 2σ < r_c) in green, and the position of the cluster centre denoted with a blue cross. Cluster members consistent with traceback to the core radius that match with the Gaia DR3 varYSO catalogue (Marton et al. 2023) are plotted with X’s. Bottom: position angle (°) around the cluster centre from the direction of increasing Galactic longitude for λ Ori cluster members that traceback to within the core radius (CA < r_c) in red, members that traceback to the core radius within 1σ (CA − σ < r_c) in yellow, and members that traceback to the core radius within 2σ (CA − 2σ < r_c) in green against a timescale of 2D traceback to the point of closest approach to the cluster centre τ_kin,CA. Cluster members consistent with traceback to the core radius that match with the Gaia DR3 varYSO catalogue (Marton et al. 2023) are plotted with X’s.