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Fig. 7


Reconstructions of the three Galaxy models with fluctuation strengths using 5000 pulsars. All panels show top-down views of the electron density in the Galactic plane using a linear color scale in units of cm-3. The panels span 36 000 pc in each dimension. The rows show reconstructions with distance errors of 15% and 5% (from top to bottom). Bottom row: original Galaxy models. Columns: reconstructions and original input models (modified NE2001) with weak, medium, and strong fluctuations (from left to right).

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