EDIBLES UVES spectra of HD 170740 (B2 V) for each setting from top to bottom: 346B, 437B, 564L, 564U, 860L, 860U. This overview figure is a demonstration of the data quality. The main gaps in wavelength coverage are between 5610–5670 Å and 8530–8680 Å which correspond to the physical separation of the Red-L and Red-U detectors in both the 564 and 860-nm settings. Note also the inter-order gaps, several are indicated with arrows, in the 860-nm Red-U spectrum above ~9600 Å as well as several conspicuous regions containing bands of closely-spaced telluric absorption lines (indicated with red horizontal bars) mostly in the Red-L and Red-U 860-nm spectra (bottom two panels). Two order-merging jumps are indicated in the fourth panel. A more detailed version of this figure is shown in Fig. B.1 where specific interstellar species are labeled and a synthetic DIB spectrum is shown for comparison.