Fig. 5.
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Observed NIRSpec spectra divided by their stellar continuum (blue), with the best-fit model (orange) for galaxies 11142 and 16874. The blue shadow is the flux uncertainty. For each galaxy the left panel shows the Ca II K, H absorption and Hϵ emission, while the right panel shows the Na I D absorption and He I emission. The dashed vertical lines mark the systemic wavelength of the absorption lines.
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