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Fitting orbits, streams and Milky Way potentials to model a large range of observables including stellar streams, rotation curve and the stars at the Galactic centre.

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GD-1 stream on a MW with a fermionic DM halo.

It is possible to reproduce the paper results. For that please go to the directory /pipeline_paper/ and follow the guidelines in the README.md there.

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Fitting orbits, streams and Milky Way potentials to model a large range of observables including stellar streams, rotation curve and the stars at the Galactic centre.

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