Fig. 9.

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Median sky density, distance, metallicity, and extinction maps (from top to bottom) of the Magellanic Clouds as seen by StarHorse (in equatorial coordinates and only including objects with dist50 > 25 kpc). Left panels: centred on the LMC, right panels: on the SMC. The contour lines in each of the panels are derived from the sky density plots in the top panels. For the LMC, the contours are drawn at stellar densities of [100, 300, 700] per pixel (from outside inwards), with 905 205 sources within the outermost contour. For the SMC, the contour lines correspond to levels [10, 50, 200], with 195 634 sources contained inside the outermost contour.
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