We report on high-resolution measurements of the photoinduced L 1 M 2 and L 1 M 3 x-ray emission lines of 69 Tm, 70 Yb, 71 Lu, 73 Ta, 74 W, 75 Re, 77 Ir, 81 Tl, 83 Bi, and 95 Am. From the linewidths of the measured transitions an accurate set of M 2 and M 3 level widths is determined assuming for the L 1 level widths the values reported by Raboud [P.-A. Raboud et al.,Phys. Rev. A 65, 022512 (2002)]. Furthermore, the present experimental M 2,3 data set is extended to 80 Hg, 90 Th, and 92 U, using former L 1 M 2,3 high-resolution x-ray emission spectroscopy measurements performed by our group. A detailed comparison of the M 2 and M 3 level widths determined in the present work with those recommended by Campbell and Papp [J. L. Campbell and T. Papp, At. Data Nucl. Data Tables 77, 1 (2001)] and other available experimental data as well as theoretical predictions is done. The observed abrupt changes of the M 2,3 level widths versus atomic number Z can be explained satisfactorily by the cutoffs and onsets of the M 2 M 4 N 1 , respectively M 3 M 4 N 3,4,5 and M 3 M 5 N 2,3 Coster-Kronig transitions deduced from the semiempirical (Z + 1) approximation. As a spin-off result of this study, precise L 1 M 2 and L 1 M 3 transition energies are obtained for the investigated elements. A very good agreement with transition energies calculated within the many-body perturbation theory is found.