Fig. 3

NIR DIBs at 10 780 Å (Groh et al. 2007) are shown for the reddened X-Shooter sample of sightlines. The spectra have been corrected for the presence of telluric lines and subsequently for the radial velocity of the ISM. The dashed lines indicate the rest wavelength for the respective DIB. Solid green curves show the Gaussian model fits and the blue solid curve displays the telluric model spectrum.
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