New GC Gran 1 as detected in the plane of the sky (upper left), in the VPD (lower left), and in the dereddened CMD (right). All data are from VVV, using the dereddened PSF photometry by Surot et al. (2019) and the PMs from Contreras Ramos et al. (2017). Small, light gray dots are field stars within 5 arcmin from the cluster center given in Table 1, while large orange dots are bona fide cluster members. Blank stripes in the upper left panel denote the chip separations where stars were rejected because the PM values were not well constrained (Contreras Ramos et al. 2017).