B-V color and A_V shown for V-band measurements determined from Gaia. B–V shows a slight increase with increasing V-band magnitude. The reported A_V follows from A_V = R_{V *} E(B–V) where E(B–V) is determined by comparing the observed B–V to the intrinsic (B–V)₀ of 0.597 mag (interpolated from table 6 in Pecaut & Mamajek (2013) for a star of 5900 K) and also increases with an increasing V-band measurement. The A_V values are slightly higher than determined by the SED fit.