Fig. 8
Influence of flaring spectra for V2689 Ori. Top panel: index time series of I(H α) with (cyan) and without (black) flare-flagged spectra. Bottom panel: comparison of the GLS with inclusion of flare-contaminated spectra (cyan/dashed) and without (black/solid). The horizontal blue lines show the FAP levels of 0.1 (dash-dotted), 0.05 (dashed), and 0.01 (solid).
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