Notes. The columns show the cluster name, the equatorial coordinates α and δ in decimal degrees, the angular radius r₅₀ enclosing 50% of the cluster members, the number N_0.7 of cluster members having a membership probability larger than 0.7, the extinction coefficient A_V, the V -band apparent magnitude m_V,⊙ of a cluster star having the Sun’s absolute magnitude M(V) = 4.83, the distance d in parsecs, and the best-fit age in Myr. The table is sorted by increasing m_V,⊙. All the parameters except for m_V,⊙ are extracted from Cantat-Gaudin et al. (2020).