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Fig. 28
Distribution of ϖTGAS/ϖRAVE−1 for ~ 200 000 stars matched in the RAVE catalogue to the TGAS solution. Stars along EPSL, λ ~ 180°, appear to have a systematically overestimated parallax of up to ~ 0.3 mas; stars with G magnitudes in the range 10−11.5 and colour 1.4 ≤ GBP−GRP ≤ 1.8 are the most strongly affected.
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