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Fig. D.13.

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Solutions for and ε* for various boundary conditions, ε, for the galaxy NGC 2403 assuming the best-fit Q* for SFDM. Top: Quantity at z = 0. The solid black line shows the minimum possible value of allowed by the condition ρSF > 0 at each radius. The smallest boundary condition, ε = 0.08, corresponds to the minimum possible dark matter mass for the given baryonic mass distribution. Smaller masses would require that the condition ρSF > 0 is violated before R = Rmax. Bottom: Same as the top panel but showing ε* instead of . The minimum possible ε* allowed by ρSF > 0 is a constant.

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