“…The weaker, hom e bui l t pro b e dye l aser (Li ttm an-t yp e design [12], spectra l wi dth about 1 cm À 1 , pum p ed synchro no usly by the same exci mer l aser), was opera ted wi th a Rho da mi ne 6G / 110 mi xture, and was set at a Ùxed wa velength resona nt wi th a few ro vi bro ni c tra nsiti ons i n the B 1 Î ê X 1 Ï + system of KLi , kno wn f rom our previ ous hi gh resol uti on studi es [7,8], thus l ab ell i ng selected ro vi bra ti ona l levels i n the gro und sta te. For perm anent contro l of the pro b e l aser frequency duri ng the m easurem ents, we ha ve chosen eight Ùxed wavel engths coi nci di ng wi th stro ng opto gal vani c l ines o f arg on.…”