Color–magnitude and radial-velocity diagrams of G vs. G_BP-G_RP from Gaia photometry. Gray points represent ωCen members with high-quality photometry, while black dots indicate the RGB stars with available APOGEE abundances, who reach up to ~30 arcmin radius. The inset shows the ΔDEC vs. ΔRA position respect to the cluster center (in arcmin) of the stars shown in the CMD. The top panel displays the radial velocity histogram of the selected sample of stars.