Fig. 5.
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Panel (a), top: Example of the best fit (in red) applied to the entire LEGA-C spectrum of the LEGA-C ID 209466 galaxy (in black). Panel (a), bottom: Difference between the observed spectrum and the best fit, shown in green, and the relative uncertainties of the observed spectrum, shown in yellow. Panel (b): Observed photometric measurements (blue points), best-fitting template (in red), and photometric measurements on the best-fitting template (lime stars). The green shaded region indicates the 68% confidence interval of our posterior.
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