Fig. C.1.

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[X/Fe] versus [Fe/H] (for O, Na, Al, and Si) for the observed sample (blue circles). The young stars are shown as green dots inside black circles, and the PISN candidates are shown as light-blue dots inside black squares. The comparison samples are the more metal-poor FS sample from (Cayrel et al. 2004, red squares) and the sample of similar metallicity from (Caffau et al. 2023, violet squares).
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