Fig. B.1.

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Overview of our analysis procedure on the whole catalog, which contains 123 076 271 stars. The top panels present observed CMDs, with the left and right panels showing the input data and their median predictions, respectively. The lower panels show the inverse parallax distance-corrected CMD and the distance corrections obtained from the AP estimates. The quantities on the y axes of these two panels would be identical in the absence of parallax noise.
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