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Fig. 2


Power spectrum of the NE2001 field without local features, clumps, and voids compared to the three unenhanced Galaxy models. The thick solid line depicts the NE2001 spectrum, the thin dashed lines depict the spectra of the models with strong, medium, and weak fluctuations (from top to bottom). To calculate the spectra, the density peak in the Galactic center is masked.

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