Fixed-physical-radius slope and full-profile comparisons of NIHAO/FIRE-2 satellites to 16 MW dwarfs show mass-dependent core formation and agreement within ~1σ for most systems, outperforming NFW.
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Dark matter density profiles of the Milky Way satellite population: reconciling simulations and observations
Fixed-physical-radius slope and full-profile comparisons of NIHAO/FIRE-2 satellites to 16 MW dwarfs show mass-dependent core formation and agreement within ~1σ for most systems, outperforming NFW.