Fig B.3.
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TESS light curve and measurements of Hα observations of the Be star λ Pav, similar to Fig. 5. The red points are from NRES, and purple from the CHIRON spectrograph. Bottom-right panel: Zoom in on the Hα EWV/EWR values fit by Eq. 2. The orange and green dots correspond to the orange and green line profiles in the upper-right panel.
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