Fig. 14.

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Results of Schwarzschild modeling of the Fornax dSph. In rows: derived mass-to-light ratio, total density, total mass, and anisotropy parameter. In columns: results for all stars and the populations, respectively. Green lines indicate the values for the best-fit models whereas the colored areas of decreasing intensity show the 1, 2, and 3σ confidence regions. The best-fitting values obtained by Kowalczyk et al. (2019) are shown with black dashed lines.
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