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Fig. 5

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Comparison of our results for Teff (left column) and log g (right column) from Run A (top), Run C (middle), and Run C2 (bottom) with interferometric radii from Boyajian et al. (2012), von Braun et al. (2014), Newton et al. (2015), and Rabus et al. (2019). If more than one value exists for a star in literature, we plot the mean with the RMSE for better readability. Results from ODUSSEAS in Run C correspond to their Run C*. The black line indicates the 1:1 relationship.

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