Fig. B.2.
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Plot of the relationship between Hα from Gaia DR3 including the model (see Eq. A.1) and logProt across (G - GRP)) colour from Gaia DR3, presented as a compliment our analyses in discrepancies between EW Hα measured by ESP-ELS in Gaia DR3 and the values reported in literature. Left: Rotation period distribution with (G - GRP)) colour-coded by normalised Hα equivalent width. Right: Hα equivalent width against (G - GRP), colour-coded by logProt. Stars with newly determined periods Prot are plotted as circles with lime-green edges, field stars in the sample are represented as circles with blue edges. The M-dwarf activity boundary plotted as dashed line follows Kiman et al. (2021)
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