Fig. 3.
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Best-fit ε values versus the best-fit Q* values for the q = 1 galaxies. We show log10|ε| rather than log10|ε − εmin| to show how many galaxies end up in the MOND limit (corresponding to |ε*|≪1) rather than how many galaxies end up close to ρSF = 0 (corresponding to |ε* − εmin|≪1). For standard SFDM, the correlation coefficient is r = 0.28.
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