The reference for most of the data no longer works, and some things are not clear, such as why there is such a big difference between going from EML2 to LEO versus going from EML1 to LEO. The figure for LEO to EML2 comes from a paper by Robert W. Farquhar. (One could probably use a similar tactic to get to EML1 for about the same delta-v.) Note that getting to one of the Lagrange points means not just getting to the right place but also adjusting the final velocity in order to stay there. Another source gives values from LEO to GEO, EML1, and lunar surface.