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Fig. 2


Distribution of VMC sources over tile SMC 5_2 as a function of distance along the x-axis (top) and the y-axis (bottom) from the centre of 47 Tuc. Bins are 1′ wide and vertical lines indicate areas dominated by 47 Tuc and SMC stars, respectively. Foreground and background sources have not been subtracted, but their distribution is more or less constant at all radii.

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