Fig. 16.

Venn diagrams with the main properties of our sample. Left: number of stars with available TESS light curve, age estimate and calculated Hα EW from the whole sample of 339 stars. Right: number of stars with detected period, flaring, and Hα emission (where the EW is at least 1σ above zero), only for the 248 stars with available TESS observation.
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