Using neural likelihood emulation on N-body simulations, the precise shape of a tidally perturbed dwarf galaxy's line-of-sight velocity field can constrain its orbit and mass profile, at least for mock galaxies.
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Using simulation based inference on tidally perturbed dwarf galaxies: the dynamics of NGC205
Using neural likelihood emulation on N-body simulations, the precise shape of a tidally perturbed dwarf galaxy's line-of-sight velocity field can constrain its orbit and mass profile, at least for mock galaxies.