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We have carried out a large-scale investigation of the metallicity and kinematics for a number of LMC and SMC star clusters using Ca ii triplet spectra obtained at the VLT. Our sample includes 28 LMC and 16 SMC clusters, covering a wide range of ages and spatial extent of the host galaxy. We determine mean cluster velocities to about 2 km s −1 and metallicities to 0.05 dex (random error), from about 7 members per cluster. Herein we present the main results for this study for the clusterdoi:10.1017/s1743921308028597 fatcat:ts44zsr37beqrcuqegw3p7up2e