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Fig. A.1.


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Radial intensity profiles from each of the six dSph galaxies: 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 flux density from a fake source. The individual flux densities are listed in Table 2. The dashed lines show the best-fitting Gaussians with a FWHM of r. The half-light radii are listed in Table 1.

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