We present Gemini South GMOS g,i photometry of 14 intermediate-age Large Magellanic 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 a continuing project to investigate the extended Main Sequence Turnoff ( EMSTO ) phenomenon .
Extensive artificial star tests were made over the observed field of view .
These tests reveal the observed behaviour of photometric errors with magnitude and crowding .
The cluster stellar density radial profiles were traced from star counts over the extent of the observed field .
We adopt cluster radii and build colour-magnitude diagrams ( CMDs ) with cluster features clearly identified .
We used the cluster ( g,g - i ) CMDs to estimate ages from the matching of theoretical isochrones .
The studied LMC clusters are confirmed to be intermediate-age clusters , which range in age 9.10 < log ( t ) < 9.60 .
NGC 2162 and NGC 2249 look like new EMSTO candidates , in addition to NGC 2209 , on the basis of having dual red clumps .