Age determination of six intermediate-age Small Magellanic Cloud star clusters with HST/ACS

We present a photometric analysis of the star clusters Lindsay 1, Kron 3, NGC339, NGC416, Lindsay 38, and NGC419 in the Small Magellanic Cloud (SMC), observed with the Hubble Space Telescope Advanced Camera for Surveys (ACS) in the F555W and F814W filters. Our color-magnitude diagrams (CMDs) extend similar to 3.5 mag deeper than the main-sequence turnoff points, deeper than any previous data. Cluster ages were derived using three different isochrone models: Padova, Teramo, and Dartmouth, which are all available in the ACS photometric system. Fitting observed ridgelines for each cluster, we provide a homogeneous and unique set of low-metallicity, single-age fiducial isochrones. The cluster CMDs are best approximated by the Dartmouth isochrones for all clusters, except for NGC419 where the Padova isochrones provided the best fit. Using Dartmouth isochrones we derive ages of 7.5 +/- 0.5 Gyr ( Lindsay 1), 6.5 +/- 0.5 Gyr ( Kron 3), 6 +/- 0.5 Gyr ( NGC 339), 6 +/- 0.5 Gyr ( NGC 416), and 6.5 +/- 0.5 Gyr ( Lindsay 38). The CMD of NGC419 shows several main-sequence turnoffs, which belong to the cluster and to the SMC field. We thus derive an age range of 1.2-1.6 Gyr for NGC419. We confirm that the SMC contains several intermediate-age populous star clusters with ages unlike those of the Large Magellanic Cloud and the Milky Way. Interestingly, our intermediate-age star clusters have a metallicity spread of similar to 0.6 dex, which demonstrates that the SMC does not have a smooth, monotonic age-metallicity relation. We find an indication for centrally-concentrated blue straggler star candidates in NGC416, while these are not present for the other clusters. Using the red clump magnitudes, we find that the closest cluster, NGC419 (similar to 50 kpc), and the farthest cluster, Lindsay 38 (similar to 67 kpc), have a relative distance of similar to 17 kpc, which confirms the large depth of the SMC. The three oldest SMC clusters ( NGC 121, Lindsay 1, and Kron 3) lie in the northwestern part of the SMC, while the youngest ( NGC419) is located near the SMC main body.