Fig. 8
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Relation between peak flare amplitude in the TESS band, ΔLf,t, and SpT. The minimum value of ΔLf,t that could be detected for each target is represented by a “_” marker. The gray dashed line marks the highest of the flare amplitude detection thresholds for all flaring stars in this sample of Lmax,th = 3.4 × 1029 erg s−1 (see Sect. 4.4). The color code visualizes the expected correlation between Lqui,T and SpT.
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