Comparison between our average reflected spectrum (solid line) and the stellar spectra from Kleinmann & Hall (1986, red dotted lines). In the left panels we show enlargement around the lines of Fe I, Ca I, and Mg I (the wavelength of each feature is marked with a vertical green dotted line), and on the right side we show the full wavelength range of our spectrum, and the name and spectral type of the stars are marked in the right side panels.