Fig. 9

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IE versus IE-HE color-magnitude diagram of all sources within the FoV of NGC 6822 after applying the selection cuts described in Sect. 5.1 and illustrated in Fig. 8 and after correction for foreground extinction (Sect. 5.2). Yellow points indicate bright MW and background galaxy contaminants, namely sources cross-matched with the Gaia DR3 catalog that have a measured proper motion PM larger than 3σPM. The vertical feature at IE - HE ≃ 1.3, IE ≳ 21 is due to the M dwarf population of the MW.
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