“…The measurements have led to extensive new information on isomers in a range of nuclei near stability and also somewhat neutron-rich, as depicted schematically in figure 24. Analysis of these data continues but details of completed results are published in a series of papers [33,67,74,94,126,128,129,130,443,444,445,446,447,448,449,450,451]. They cover a broad range in terms of physics, from the characterisation of comprehensive multi-quasiparticle isomers in 174 Yb [445], for example, to the identification of transitions to intermediate states that could connect the high-K and low-K isomeric and ground states in 176 Lu by photoexcitation, thus affecting elemental abundances in a stellar environment [33].…”