Left: proper motion diagram of the NGC 3532 stars with the recovered and literature WD proper motion overlaid. Cluster stars with cluster membership probability < 0.5 are marked using gray crosses, while black crosses indicate likely cluster members. Here, and in the subsequent graphs, the errorbars indicate a 1σ uncertainty, as reported in the GDR2. Errorbars for the cluster stars are omitted for clarity. Middle: parallax histogram of the cluster member stars (membership probability ≥0.5) with WD parallaxes overlaid. Right: cluster member star CMD with WDs overlaid.