Our visible and NIR spectropolarimetric measurements of the earthshine compared to literature data. A 10-pixel binning was applied to the NIR spectrum of region B. The uncertainty per wavelength is plotted as vertical gray error bars. Wavelengths of strong telluric absorption have been removed. Some molecular species seen in “emission” (indicative of strong atmospheric flux absorption and less multiscattering processes occurring at those particular wavelengths) are labeled. The vertical dashed line separates the ALFOSC and LIRIS data.