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Halometry---mapping out the spectrum, location, and kinematics of nonluminous structures inside the Galactic halo---can be realized via variable weak gravitational lensing of the apparent motions of stars and other luminous background sources.
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F. C. van den Bosch and G. Ogiya, Dark matter substructure in numerical simulations: A tale of discreteness noise, runaway instabilities, and artificial disruption , Monthly Notices of the Royal Astronomical Society (2018)
2018
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