Figure 2
Φcosmo as a function of the angle of view ψ from the centre of halo, computed in the case of Draco, for the smooth halo and from the subhalo population. The shaded region represents the uncertainty due to the numerical simulations in the value of Φcosmo computed for the MW, including its substructures, at the position of Draco.

Φcosmo as a function of the angle of view ψ from the centre of halo, computed in the case of Draco, for the smooth halo and from the subhalo population. The shaded region represents the uncertainty due to the numerical simulations in the value of Φcosmo computed for the MW, including its substructures, at the position of Draco.

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