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Fig. 1.

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Bias in different distance estimates. Left: GSP-Phot heliocentric distances as a function of parallax inverse. The colour bar shows the mean parallax quality inside each pixel. The quality cut used in this paper corresponds to log10(ϖ/σϖ) > 1.301. Right: same but for photogeo heliocentric distances by Bailer-Jones et al. (2021).

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