Spectral region around the LiI λ670.78 nm line is shown for the sample of stars newly observed at OHP, NOT, and Keck. All spectra were flux normalized to unity at the nearby continuum and were boxcar smoothed with a 10-pixel wide filter for clarity (corresponding to 0.01, 0.025, and 0.03 nm for OHP, NOT, and Keck spectra, respectively). The vertical dotted line corresponds to the central wavelength of the LiI 670.78 nm line profile shifted by +5.6 km/s, the average radial velocity of Pleiades cluster members (Galli et al. 2017).