FEROS spectra of targets in the Eagle region and the Lagoon Nebula. Wavelengths were shifted to the rest position of the K I line (top) component corresponding to the motion of the local ISM. The middle panel shows the profile of the 6196 Å DIB. The bottom panel shows the same feature with intensities scaled to the same line depth. Continuum normalisation was not applied when producing this figure the fluxes were only re-scaled using the median of the flux within 5 Å from the shown features.