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Dark Matter and MOND successes and degeneracies in reproducing SPARC rotation curves and weak lensing data
The observed rotation velocities of spiral galaxies at large scales exceed those predicted by their baryonic components, motivating the need for dark matter (DM) or Modified Newtonian Dynamics (MOND). We fit the rotation curves of 147 late-type galaxies from the SPARC database, using a suite of mode
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