Left: color–magnitude diagram of NGC 6802 stars. The background dots are photometric data from Janes & Hoq (2011). Stars with photometric membership probability greater than 50% are shown as gray filled circles. We also plot the UVES cluster members (magenta filled circles), UVES non-members (magenta crosses), GIRAFFE LMS (lower main sequence) cluster members (green filled circles), GIRAFFE LMS non-members (green crosses), GIRAFFE UMS (upper main sequence) cluster members (blue filled circles), and GIRAFFE UMS non-members (blue crosses). Empty circles indicate UMS stars with RV between 18 and 21 km s^-1. The symbol meanings are also applicable to the other panels. Top right: locations of stars observed by Janes & Hoq (2011), UVES, and GIRAFFE. Bottom right: distance from the cluster center as a function of radial velocity. The median radial velocity of the GIRAFFE members is marked as a solid line.