UVES spectra of DIB at 6284 Å toward SMC (left) and LMC (right) stars observed under program V03. The vertical scale is expanded by a factor of 10. Letters "G," "S," and "L" mark velocities of strongest Galactic, SMC, and LMC Na I absorption, respectively. The weak feature near 580 km s⁻¹ is a residual instrumental artifact; telluric emission lines may be noted near 150 and 760 km s⁻¹ (truncated).