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Fig. 5.

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C3He2 versus C43 diagnostic diagrams, selecting only one NLAGN due to the difficulties in detecting rest-UV lines in high-z galaxies with the short exposure times of the CEERS survey. The stacking line ratios and the average errors are not reported because of the poor statistics. The colors follow the same scheme as in Fig. 2. The demarcation lines are those defined in Hirschmann et al. (2023).

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