Potamides: Mapping Dark Matter Halo Shapes from Stellar Stream Tracks in the Local Universe
Sirui Wu, Nathaniel Starkman, Sarah Pearson, Jacob Nibauer, Juan Miro-Carretero, David Martinez-Delgado

TL;DR
Potamides uses stellar stream curvature to constrain dark matter halo shapes in external galaxies, providing a new observational method to test dark matter models and galaxy formation theories.
Contribution
The paper introduces Potamides, a novel technique leveraging stellar stream curvature to infer dark matter halo shapes around external galaxies.
Findings
Some streams exclude large halo flattening regions.
Edge-on wrapping streams give strong shape constraints.
All streams support spherical halos for a given flattening direction.
Abstract
Stellar streams trace the gravitational potential of their host galaxies and offer a direct probe of dark matter halo geometry. Cosmological simulations predict that halo shapes depend on both baryonic physics and the nature of dark matter, yet observational constraints on halo flattening and orientation remain limited, especially for individual galaxies. We present Potamides, which utilizes the curvature of extragalactic stellar streams to derive constraints on halo shapes. We apply Potamides to 15 stellar streams from the Stellar Stream Legacy Survey to infer the projected axis ratios and orientation of their host halos. We find that some streams in our sample exclude large regions of halo flattenings and halo orientations. Systems with edge-on wrapping loops or sharp turning points yield the strongest constraints, whereas great circle-like streams remain largely uninformative. All…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
