Fig. A.1.
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Comparison of EW Hα from Gaia DR3 and literature. Left panel: For the sample of stars, three values of equivalent width of Balmer α line were plotted according to Eq.A.1: Gaia DR3 EW Hα, Gaia DR3 EW Hα with added model and EW Hα found in literature. Right panel: the diagram presents the effect of the model from the relation described in Eq.A.1. Ages of the sample’s stars are colour-coded from youngest (blue) to oldest (yellow).
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