Fig. 11.
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Individual elemental abundance differences for APOGEE−GALAH (bottom), APOGEE−GES (middle), and GALAH−GES (top) common samples relative to hydrogen (left column) and on an absolute scale (right column). The shaded interval accounts for a ±0.1 dex range. The calculated results for GB and MS stars are shown as filled red and empty black circles, respectively.
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