Axisymmetric models of Draco and Ursa Minor find a cuspy dark matter halo in Draco, a cored one in Ursa Minor, and no evidence for intermediate-mass black holes.
Each MCMC run is post-processed to ensure that the retained samples are independent and representative of the converged posterior
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Multi-component, axisymmetric dynamical models of dSphs based on distribution functions: inferences on dark matter and intermediate-mass black holes in Draco and Ursa Minor
Axisymmetric models of Draco and Ursa Minor find a cuspy dark matter halo in Draco, a cored one in Ursa Minor, and no evidence for intermediate-mass black holes.