GraphNPE recovers a significantly lower central density for Boötes I consistent with a core while Draco remains marginally cuspy, and demonstrates that higher-order velocity moments reduce bias in dynamical modeling.
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HST astrometry on archival baselines can deliver full 3D kinematics and internal motions for Local Group galaxies, streams, and clusters, supporting dynamical studies of orbital histories and dark-matter structure.
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Dark Matter in Draco and Bo\"otes I: Hints of a Core in an Ultra-Faint Dwarf from Simulation-Based Inference
GraphNPE recovers a significantly lower central density for Boötes I consistent with a core while Draco remains marginally cuspy, and demonstrates that higher-order velocity moments reduce bias in dynamical modeling.
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Hubble Astrometry for the Local Group and Beyond in the 2030s
HST astrometry on archival baselines can deliver full 3D kinematics and internal motions for Local Group galaxies, streams, and clusters, supporting dynamical studies of orbital histories and dark-matter structure.