Fig. 1
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Distributions of the G magnitudes of the GES parent sample (𝒮0; blue), of the GES stars having a Gaia DR3 radial velocity (𝒮1; orange), and of the Gaia-ESO stars having the three main Gaia GSP-Spec atmospheric parameters (𝒮3; green). The bin positions and width are identical for the three histograms; the bin width was adjusted using the Freedman-Diaconis rule.
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