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Published online by Cambridge University Press: 30 October 2025
The Small Magellanic Cloud (SMC), as one of the nearest galaxies to us, provides a superb laboratory for studying resolved stars in exquisite detail. We present here the largest sample of SMC Red Giant Branch (RGB) stars (∼6000) observed with the AAOmega spectrograph fed by the Two Degree Field (2dF) multi-object system at the Anglo-Australian Telescope of the Siding Spring Observatory (Australia). Metallicities were recovered using a direct estimation of [Fe/H] from the equivalent widths of the Calcium triplet (CaT). We discuss the potential implications of the metallicity gradients and compare them with previous determinations of star formation history to assess the consequences of encounters between the SMC and the Large Magellanic Cloud.