Flying far and fast: the distribution of distant hypervelocity star candidates from Gaia DR2 data

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Fig. 3.

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Extinction and reddening, a comparison. Left panels: extinction values A_V from Schlegel et al. (1998), (top panels), and Schlafly & Finkbeiner (2011), (bottom panels), versus the line-of-sight extinction A_G from Gaia DR2 for the 15 681 sources in our primary sample (in grey) and the 393 stars with the best astrometric solutions (in black). Right panels: colour excesses E(B − V) from Schlegel et al. (1998) and Schlafly & Finkbeiner (2011) versus E(G_BP − G_RP) from Gaia DR2 for the same sources. The reference line in red is the diagonal. See the text for additional details.

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