Stellar spectra from ESO observing program 084.B-0869(A). All stars were observed on the night of 2009 November 26 and automatically extracted with the prescriptions presented in this work. Each target was observed in NOD mode with a slit width of 0.5″. The underlying sensitivity functions were derived with the spectrophotometric standard star GD 71. The three panels cover the spectral type range from a hot star with spectral type A3 (top panel), to an intermediate-type star F8 (middle panel), to a cool giant star with a spectral type K3 (bottom panel).