O abundances as functions of effective temperature (upper panel) and against Al abundances for three of our clusters (bottom panels) determined by the BACCHUS code with the APOGEE DR14 uncalibrated Teff and log g (black dots) and by the ASPCAP pipeline (uncalibrated values, red triangles). The oxygen trend is slightly positive in contrast to Fig. 7. Moreover, almost no O dispersion nor anticorrelation is observed, which cast some doubts on the stellar parameters.
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