Fig. 2
Examples of the local renormalization for five RAVE spectra (R = 7500) of hot stars. The black lines are the original spectra, and the orange lines indicate the renormalized spectra. The black arrows indicate the Gaia DIB. The names and atmospheric parameters are also indicated. The strong stellar feature near the DIB profile seen on HD 150850 and HD 166167 is the N I line.
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