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The missing ultra-faint satellites of the Milky Way
We combine the highest resolution N-body simulation of a $\sim10^{12}M_\odot$ $Λ$CDM halo (Aquarius-A) with the semi-analytic model GALFORM to study the full satellite population of Milky Way (MW)-like galaxies. The model assumes that galaxies form only in subhalos whose peak circular velocity excee
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