Measurements of projected rotational velocities and the rotational profile of stars with spectral types A-F are presented. This work completes previous measurements by line profile analysis. New spectra with high signal-to-noise ratio were taken with the high-resolution CES and FEROS spectrographs operated by ESO at La Silla, Chile. Stellar rotation is studied in inverse wavelength space analysing the first two zeros of the Fourier transform of the overall broadening profile. Rigid and differential rotation can be distinguished in the case of rapid rotation. New and previous measurements are compiled and made available. The data are supplemented by a homogeneous compilation of basic stellar data from photometry. Data are flagged when there are indications of multiplicity.