Abstract
The wave functions derived by Kisslinger and Sorensen from the pairing plus quadrupole force model for atomic nuclei are used to compute theoretical E2 electromagnetic transition rates between various low-lying states in odd-mass spherical nuclei from Ni to Pb. Comparison is made with experimental data where available. The agreement between theory and experiment is quite good, a large majority of the forty or so cases agreeing within a factor of 2 while the data cover a range of more than a factor of 1000.