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Fig. 6


Recovered Galactic profile in the Galactic plane. Shown is a top-down view the Galaxy as in Fig. 5, but here in logarithmic color scale. The input model had medium strength fluctuations, it was recovered using 5000 pulsars with 5% distance uncertainty (corresponding to the bottom middle panel in Fig. 5). Other fluctuation strengths and data sets would yield a very similar image.

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