Fig. 2.

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Composite color image of Leo T based on data from the MUSE-Faint survey, created with fits2comp (https://github.com/slzoutendijk/fits2comp). We used the Johnson-Cousins filters I, R, and V to create the red, green, and blue channels of the image, respectively. The 58 stars identified in this paper as Leo T members that are located within the bounds of MUSE-Faint observations are identified with circles. As we identify two stellar populations (see Sect. 4.1), we use blue and red circles for the younger and older population, respectively. The angular and physical scales of the image are indicated in the lower left corner. Directions north and east are indicated in the lower right corner of the image.
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