Figure 2.
Observed spectra (in black) and selected clean stellar lines (red) for calculating the residual distortion. A Gaussian fit to the lines is shown in red. A zoomed version of a Gaussian fit is shown in the subplot.
Observed spectra (in black) and selected clean stellar lines (red) for calculating the residual distortion. A Gaussian fit to the lines is shown in red. A zoomed version of a Gaussian fit is shown in the subplot.
