Fig. 1.
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JWST/NIRSpec Prism 1D spectroscopy of the sample, shown in shades of blue, with the associated error spectrum as a shaded region. The positions of the main line transitions are highlighted by grey lines. The inset zooms in on the spectroscopically resolved Hγ + [O III] λ4363 emission lines, with the best-fit continuum and emission-line model for each galaxy shown by the pink lines.
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