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Fig. A.1

Fig. A.1 Refer to the following caption and surrounding text.

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Comparison with OCs and GCs samples. We show the mean cluster abundance ratios as a function of [Fe/H], with the main aim to compare the chemistry of Patchick 126 (cyan circle) with that of old OCs from the Myers et al. (2022) compilation (brown triangles) and with GCs from Mészáros et al. (2020) (purple diamonds) at the same metallicity range. The oldest known OC, NGC 6791, is highlighted with a red star.

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