“…Until 1972 STKr decay [1,2] was the source of most of the level structure of SVRb. Since then, (n,n'7) [3,4], (p,p') [5], Coulomb excitation [6], SSSr(d, 3He) [7,8], and S6Kr(3He, d) [9,10] experiments have confirmed much of the early structure information and added new information. As a result of these experiments, the energy levels of STRb and the spins, parities, and spectroscopic factors for the lowest lying levels have become reasonably well known.…”