Fig. 7.
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Stacked histogram of the number of stars in bins of 200 pc for the final sample of stars up to 4000 pc. The distances were obtained either from Bailer-Jones et al. (2021; blue bins) or using the inverse of the parallax from HIPPARCOS for stars without Gaia DR3 data (orange bins). The latter are limited to those with σϖ/ϖ ≤ 0.1.
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