Additional constraints on the parameter pairs (M₃₄₀,c) coming from studies from the literature. The black contours are the same as in Fig. 13. Gnedin et al. (2010) measured the mass interior to 80 kpc from the GC, Xue et al. (2008) within 60 kpc and Kafle et al. (2012) inside 25 kpc. The yellow solid and dotted line separate models for which the satellite galaxy Leo I is on a bound orbit (below the lines) from those where it is unbound.