Standard strong-lensing mass models over-estimate dark matter; observations without them directly constrain only local properties of the deflecting mass.
ApJ973(1), 61 (2024)
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Review chapter on SKA observations of RELHICs and dim galaxies to constrain LambdaCDM and baryonic physics via HIMF, HIVF, and bTFR down to 10^6 solar masses.
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Standard strong-lensing mass models over-estimate dark matter; observations without them directly constrain only local properties of the deflecting mass.