Fig. 5.
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Visualization of the full spectral fit of eRASSt J1906-4850 Magellan/Baade spectrum. The observed spectrum of the galaxy is shown in black, while the pPXF best-fit stellar model is shown in red. A continuum-free emission-line spectrum is shown in green, and the individual Gaussian components are shown in blue. We show the Hβ + [O iii] complex and the Hα + [N ii] + [S ii] in the left and right panel, respectively.
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