Fig. C.2

image

Differential parallax bias estimated by means of RC stars. The plots show differences between the measured parallaxes ϖEDR3 and the photometric parallaxes ϖRC from Eq. (C.2) in area N (a) and S (b). Contours of constant density are shown as thin grey lines. The thick black curve traces the ridge of the feature created by the red clump stars.

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