Example of output single-exposure normalized spectra obtained using the ESO-pipeline (upper blue spectrum) vs. IRAF tasks (lower black spectrum), for the same target star. The two spectra were offset on purpose for direct comparison. Although the IRAF reduced spectrum presents higher residual at redder wavelengths (where we note the presence of a telluric absorption band), around the CaT it turned out to be cleaner and less noisy than the ESO-pipeline reduced one.