Gaia Data Release 2
Free Access

Fig. 30

image

Identification of the most degenerate extinction estimates for high Galactic latitude stars with |b| > 50° before applying the filters of Eqs. (8)–(10). Panels a and b show the identification via the asymmetry of confidence intervals. Panels c and d show the identification via the lower confidence interval. A corresponding plot for E(BP − RP) is provided in the online documentation.

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