Fig. 3
Diagram representing the measured WISE [4.6] magnitudes of known RCB stars versus the difference in magnitude between the WISE measurement and the best SED model found. For objects brighter than [4.6] ~ 5.0, the [4.6] WISE brightness is overestimated, reaching ~0.9 mag at [4.6] ~ 3.0 mag. The red line is a representation of this bias.
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