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Fig. 1.

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Radial profile of an FDM halo (Mh = 7 × 1011M and mψ = 10−22 eV at z = 0.9), neglecting quantum fluctuations (solid black line). The inner profile of the halo is dominated by the soliton structure (dot-dashed red line). At r = rsol, the profile transitions to a standard NFW dark matter halo (dashed blue line). The radial variance of the fluctuations, given by Eq. (21) (dot-dashed grey line) is shown in arbitrary units.

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