Distribution on the sky of the 111 GC containing stars whose radial velocities are published in Gaia DR3. The colour code indicates the number of stars with measured velocity in each cluster. The image uses an Aitoff projection in Galactic coordinates (l, b). The Galactic centre is at the centre of the image, and the Galactic longitudes increase to the left. Clusters with more than 200 members with a Gaia DR3 radial velocity are circled in black, and their names are reported on the plot.