Fig. G.1.
Total reddening observed in the optical, E(B − V)∞, as a function of E(B − V)τ, the dust optical depth at 353 GHz converted to a reddening, for the 1505 selected stars (Sect. 6.3). Each bin of the running mean contains the same number of lines of sight. Error bars represent the standard deviation in each bin. The dashed line corresponds to a one-to-one correlation.
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