Fig. 5.
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Predicted cumulative number of satellites brighter than a given luminosity, within 300 kpc of M83, assuming a mass of 0.8 × 1012 M⊙. The 1, 2, and 3σ confidence intervals are indicated with the blue areas. The black line corresponds to the LF of M 83. The vertical dashed line represents the survey limit of Müller et al. (2015). The M 83 LF deviates by more than 3σ from the subhalo mass function.
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