Panel a: same as Fig. 6, but for all correlated spectra, representing all inner disk spectral shapes. Panel b: values derived from total spectra are shown, averaged for each individual object. The solid green line is our fit to the data, the dashed line is a fit from Przygodda et al. (2003) for T Tauri stars, and the dot-dashed line is a fit from van Boekel et al. (2003) for Herbig Ae/Be stars.
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