Fig. 8
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Spatial distribution of the ɡdr3wise[RC] sample for the region considered for model fitting. Panel a shows the galactocentric XGC–YGC projection, with the location of the Sun (black star) and the Galactic centre (black dot) also indicated. Stars within R < 3kpc of the Galactic centre have been removed. Panel b shows the corresponding galactocentric YGC–ZGC projection. The number density is shown on a logarithmic scale.
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