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Spectroscopy from the final internal data release of the Gaia-ESO Survey(GES) has been combined with Gaia EDR3 to assign membership probabilities totargets observed towards 63 Galactic open clusters and 7 globular clusters. Themembership probabilities are based chiefly on maximum likelihood modelling ofthe 3D kinematics of the targets, separating them into cluster and fieldpopulations. From 43211 observed targets, 13985 are identified as highlyprobable cluster members ($P>0.9$), with an average membership probability of0.993. The addition of GES radial velocities successfully drives down thefraction of false positives and we achieve better levels of discrimination inmost clusters over the use of astrometric data alone, especially those atlarger distances. Since the membership selection is almost purely kinematic,the union of this catalogue with GES and Gaia is ideal for investigating thephotometric and chemical properties of clusters as a function of stellar mass,age and Galactic position.

The Gaia-ESO Survey: Membership probabilities for stars in 63 open and 7 globular clusters from 3D kinematics