EDIBLES spectrum for HD 170740 (solid blue). The preliminary normalisation shown here is from spline fits to broad regions of each UVES settings, and order-merging residuals can also be seen – future quantitative analysis will employ tailored, local rectifications of the data. Electronic transitions of interstellar atomic and di-atomic species are labeled. Above 4000 Å a generic model of the telluric transmission spectrum (retrieved from the ESO Sky Calculator) is shown in yellow/orange as well as the Jenniskens & Désert (1994) average ISM DIB spectrum (scaled to E(B−V) = 0.5 mag) in solid green.