Fig. B.1.
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Calibrated Gaia DR3 RVS [Fe/H] as a function of [Fe/H] estimates from GALAH DR3 (top panel) and APOGEE DR17 (bottom panel) of stars with [Fe/H] < -0.5 that pass the quality selection criteria. Small and big circles show stars before and after removing stars with Gaia DR3 RVS [Fe/H] > -2 and the fluxnoise_flag = 2, respectively. The color code indicates the [α/Fe] Gaia RVS DR3 measurements between for each star.
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