Extended Data Fig. 6: Comparison of spectral fitting results using two different methods.
From: A post-starburst pathway for the formation of massive galaxies and black holes at z > 6
The top and bottom panels show the decomposed host spectrum (light blue) for J2236 + 0032 and J1512 + 4422, respectively. The best-fit models from Bagpipes (dark blue) and pPXF (orange) are overlaid. The red wing of the Hγ absorption of J1512 + 4422, shown as gray shade, is masked in the spectral fitting.
