A self-consistent direct method for chemical abundances in high-z galaxies with JWST
The unprecedented rest-frame UV and optical coverage provided by James Webb Space Telescope (JWST) enables simultaneous constraints on the electron density ( $n_{\rm e}$) and temperature ( $T_{\rm e}$) of ionized gas in galaxies at $z\,\gt\,5$. We present a self-consistent direct method based on multiple O III] ( $\lambda \lambda$1661, 1666) and [O
Arellano-Córdova, K. Z. et al.
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4
2026