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Fig. 2.
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Halo (top) and outer disk (bottom) MUSE FoV. The images were created using the flux in the wavelength range from 6869 to 9300 Å, representative of the F814W HST/ACS filter. Red points are the RGB and AGB+RGB stars, until two magnitudes below the TRGB selected by GHOSTS in each FoV.
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