Fig. 37
Selection of target candidates for interferometry colour-coded by (a) number of stars, (b) Priam estimate of Teff, and (c) FLAME estimate of radius. The stellar angular diameter θ is plotted on a log scale. We find 213 139 candidates with angular diameter θ > 0.2mas, 95 794 candidates with θ > 0.3mas, and 52 196 candidates with θ > 0.4mas. The black dashed line in panel a corresponds to G = const − 5log10θ.
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