Interference in fuzzy dark matter filaments - Idealized models and statistics

Open Access

Fig. 3.

Radial filament densities obtained from Eq. (12) (solid lines) and the solution of the inverse problem of Eq. (17) (dashed lines), i.e., the density implied by the DF. Vertical lines depict the fit radius R₉₉ within which 99% of the total line mass μ are contained.

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