Probing the Dark Matter Halos of External Galaxies with Stellar Streams
Stellar streams have proven to be powerful tools for measuring the Milky Way’s gravitational potential and hence its dark matter (DM) halo. In the coming years, the Vera Rubin Observatory, Euclid, ARRAKIHS, and the Nancy Grace Roman Space Telescope will ...
Madison Walder +3 more
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Comment on “Modeling galaxy halos using dark matter with pressure” [PDF]
Kung-Yi Su, Pisin Chen
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Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter [PDF]
Alis J. Deason +5 more
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Line-of-sight Bias in Dark Matter Inferences from Galaxy Cluster Mergers
In collisions of galaxy clusters, the lack of displacement between dark matter and galaxies suggests that the dark matter scattering depth is small. This yields an upper limit on the dark matter cross section if the dark matter column density is known ...
David Wittman +2 more
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Three-point galaxy-galaxy lensing as a probe of dark matter halo shapes [PDF]
Susmita Adhikari +2 more
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Leaving No Branches Behind: Predicting Baryonic Properties of Galaxies from Merger Trees
Galaxies play a key role in our endeavor to understand how structure formation proceeds in the Universe. For any precision study of cosmology or galaxy formation, there is a strong demand for huge sets of realistic mock galaxy catalogs, spanning ...
Chen-Yu Chuang +4 more
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The large extent of dark matter haloes probed by the formation of tidal dwarf galaxies [PDF]
F. Bournaud +2 more
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Galaxy–dark matter connection of photometric galaxies from the HSC-SSP Survey: galaxy–galaxy lensing and the halo model [PDF]
Navin Chaurasiya +5 more
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Xu & Jing reported a monotonic relationship between the host halo mass M _h and the morphology of massive central galaxies, characterized by the Sérsic index n , at fixed stellar mass, suggesting that morphology could serve as a good secondary proxy for ...
Zhenjie Liu +4 more
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Chameleon gravity as an alternative to dark matter
By studying the chameleon gravity on galaxy scales, we investigate the effects of the chameleon dark matter. To perform this task, we consider the dynamics of the chameleon scalar field in the region of galactic halos in static spherically symmetric ...
Raziyeh Zaregonbadi +2 more
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