Present-day heliocentric Galactic Cartesian coordinates of the field star purged member candidates of the Sco-Cen complex selected by Luhman (2022), colour-coded by population. Plotted are only stars for which Gaia measurements of radial velocities are available. The maps in the background show slices (from left to right along the plane through the Sun parallel to the Galactic mid-plane, the rotation plane, and the meridian plane) of the 3D dust density distribution in the LISM based on measurements of starlight absorption by dust (Lallement et al. 2019). The colour-coding is black (light yellow) for high (low) dust densities. The dotted white contours correspond to a differential extinction of 0.003 mag pc⁻¹ and delimit dense regions that are probably related to the LB’s outer shell.