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Fig. 3
Top panel: comparison between our SBCR for early-type stars and relations of Challouf et al. (2014), Boyajian et al. (2014), Kervella et al. (2004), and Adams et al. (2018). Bottom panel: differences in angular diameter estimates between ourSBCR and the other relations. See Sect. 5.3 for more details on the comparison.
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