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We present Gemini South GMOS g,i photometry of 14 intermediate-age LargeMagellanic Cloud (LMC) star clusters, namely: NGC 2155, 2161, 2162, 2173, 2203,2209, 2213, 2231, 2249, Hodge 6, SL 244, 505, 674, and 769, as part of acontinuing project to investigate the extended Main Sequence Turnoff (EMSTO)phenomenon. Extensive artificial star tests were made over the observed fieldof view. These tests reveal the observed behaviour of photometric errors withmagnitude and crowding. The cluster stellar density radial profiles were tracedfrom star counts over the extent of the observed field. We adopt clus- terradii and build colour-magnitude diagrams (CMDs) with cluster features clearlyidentified. We used the cluster (g,g-i) CMDs to estimate ages from the matchingof theoretical isochrones. The studied LMC clusters are confirmed to beintermediate-age clusters, which range in age 9.10 < log(t) < 9.60. NGC 2162and NGC 2249 look like new EMSTO candidates, in addition to NGC 2209, on thebasis of having dual red clumps.

Gemini/GMOS photometry of intermediate-age star clusters in the Large Magellanic Cloud