Representative spectra and our fits across the range of our sample for the first quarter of our wavelength regions. For each star, the solid black line is the observation, and the dash-dotted colored line is the model. At the bottom of each subplot, the green solid region indicates pixels included in our line and continuum masks. Additional regions are removed from this mask based on the positions of telluric lines. All spectral regions are plotted at the same wavelength scale to facilitate comparisons of spectral features, though this will leave some subpanels relatively empty.