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Fig. 3.
Log–log plot of the observed counts of stars 
(with a bin width Δπ = 0.01 mas.) as a function of the parallax, together with the calculated star counts NΔπ after the deconvolution was applied, for the Gaia-DR2 with measured radial velocity and with the constraints: |ℓ−180 ° | < 20°, |b|< 10°, 
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