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We have obtained near-infrared spectra covering the Ca II triplet lines for anumber of stars associated with 16 SMC clusters using the VLT + FORS2. Thesedata compose the largest available sample of SMC clusters withspectroscopically derived abundances and velocities. Our clusters span a widerange of ages and provide good areal coverage of the galaxy. Cluster membersare selected using a combination of their positions relative to the clustercenter as well as their abundances and radial velocities. We determine meancluster velocities to typically 2.7 km/s and metallicities to 0.05 dex (randomerrors), from an average of 6.4 members per cluster. (continued in paper)

Ca II Triplet Spectroscopy of Small Magellanic Cloud Red Giants. I. Abundances and Velocities for a Sample of Clusters