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. 2023 Dec 23;527(4):12120–12139. doi: 10.1093/mnras/stad3973

Figure 3.

Figure 3.

Differential reddening ΔE(VI) deduced for spectroscopic targets, as a function of their effective temperature. The mean value −0.013 ± 0.032 mag is indicated by a solid blue line. Differential reddening values are on average slightly more negative for cooler stars (see the text for further discussion).