Fig. F.2.
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Comparison between CLOUDY-predicted RFe generated with SEDs from Jin et al. (2012, 2017) and RFe measured from observations. Models are colour-coded according to their ionisation parameters. The range of metallicities derived from narrow lines observed in JWST-selected type 1 AGNs is indicated by the vertical grey shaded region. With these SEDs constrained by observations, low metallicities are still needed to explain the low RFe in our sample of JWST-selected AGNs.
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