Orbit anisotropy of dark matter haloes with Schwarzschild modelling
  We apply the Schwarzschild orbit superposition method to mock data in order
to investigate the accuracy of recovering the profile of the orbit anisotropy.
The mock data come from four numerical realizations of dark matter haloes with
well defined anisotropy profiles. We show that when assuming a correct mass
distribution we are able to determine the anisotropy with high precision and
clearly distinguish between the models.
