VPD (left panel) and CMDs (middle and right panels) of NGC 6749 using the new HST data of the MGCS survey. The red circle with the radius of 1 mas yr⁻¹ in the VPD was used to select likely cluster stars (those included within the circle). In the central CMD, the gray dots represent all stars in our HST photometric catalog, and the black and red dots are foreground and cluster stars, respectively, for which we have a PM measurements. The horizontal dashed line corresponds to the Gaia limiting magnitude. Finally, the right panel shows the location of cluster member stars in the CMD.