Fig. 2.
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Zoom-in to the rest-frame UV part of the PRISM spectrum of CEERS-1019 (black and 1σ uncertainty in grey). Vertical dashed lines (green) mark the position of nebular emission lines. The blue line is the best fit for several UV emission lines and continuum. The bottom panel shows the residuals (in the same units as the spectrum) as well as the 1σ uncertainties (grey).
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