Fig. B.1.
Comparison of StarHorse DR16 distances to naive distances obtained by inverting the recalibrated Gaia DR2 parallaxes. Top panel: one-to-one comparison of posterior with naive 1/ϖ distances. Bottom panel: residuals between pure astrometric and spectro-photo-astrometric (1/d50) parallaxes. The red line shows the smoothed running median, while the shaded region shows the corresponding 1σ variations.
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