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Fig. 2

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Distributions of distances from different sources in the solar-like star dataset. The green, blue, and purple lines represent the distributions with ϖ/σϖ > 5, ϖ/σϖ > 10, and ϖ/σϖ > 20, respectively. Panels a, b, and c show the distributions of raw inverse parallax, geometric distances, and GSP-Phot distances. The distributions of inverse parallax with zero-point correction for different error cuts are shown as black dotted, gray dot-dashed, and silver dashed lines, respectively. For comparison, these distributions are shown in all three panels.

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