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Fig. A.2.


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Best-fitting Gaussian amplitudes for the radial intensity profiles in Figs. A.1a- A.1f: Canes Venatici I (panel a), Ursa Major I (b), Ursa Major II (c), Ursa Minor (d), Willman I (e), and Canes Venatici II (f). Blue indicates purely observational data, and red indicates data with an additional fake source. The added individual flux densities are listed in Table 2. The shaded areas are 1σ intervals.

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