Extended Data Fig. 2: Double-peaked Hα emission for J1512 + 4422.
From: A post-starburst pathway for the formation of massive galaxies and black holes at z > 6
The observed Hα profile (after continuum subtraction) is shown in black. Our model fit based on the method presented in ref. 59 is shown as colored lines (dark blue: disk model, light blue: narrow lines, red: total). The wavelength and the flux density are presented in the rest frame. The bottom panel shows the residual fluxes, that is, the difference between the observed profile and the best-fit model.
