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Fig. 1

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VISTA image of NGC 253 with the field of view of previous resolved stellar population studies from the literature over-plotted; specifically IMACS at Magellan (Bailin et al. 2011, cyan circle), 3 WIRCam at CFHT fields (Davidge 2010, large blue squares), NTT SUSI2 (Comerón et al. 2001, yellow rectangles), and many ACS fields (GHOST survey, Radburn-Smith et al. 2011, small green squares). The HST WFC2 field from Mouhcine et al. (2005a, small red square) partially overlaps with ACS, SUSI2, and IMACS fields. The wide coverage of the VISTA data can be readily appreciated.

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