Fig. 2.

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Percentage difference between Gaia EDR3 parallax and HIPPARCOS parallax (van Leeuwen 2007) with respect to Gaia EDR3 in mas. The error represents the uncertainty of EDR3 parallaxes and HIPPARCOS parallaxes propagated through the percentage difference. The open circles represent the Kepler legacy stars, the solid black circles represent Gaia-ESO stars, and the single open square represents our metal-poor star ν Ind. The average uncertainties for the Kepler legacy and Gaia ESO stars are shown in the bottom right corner.
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