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Fig. 6.

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Red clump star properties towards the Galactic poles (NGP+SGP): from top left to bottom right, distribution of ρ, ⟨Vϕ⟩, σR, and σz with respect to ϕ at four values of |z| (0.5, 1, 1.5 and 2.5 kpc) (resp. blue, grey, pink, and cyan lines).
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