Open Access

Fig. 8.

image

Radius from GRAVITY and Keck/AMBER NIR interferometry, measured relative to the empirical radius-luminosity relation from reverberation mapping (Suganuma et al. 2006; Koshida et al. 2014). Reverberation sizes are shown for comparison, and the error bars correspond to 1σ in all cases. Both interferometry data sets show a larger median size R/Rin >  1 and decreasing relative size with increasing luminosity, particularly evident as R/Rin ≲ 1 for quasars.

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