“…As a by-product of an investigation of the level structure of 45,46 Ar through in-beam γ -ray spectroscopy using the fragmentation of a 60 AMeV 48 Ca beam, Dombrádi et al [31] identified a γ -ray transition of energy 904(7) keV, which was attributed to 39 S. Thus, although the 339.9-, 398.6-, 465.5-, 904-, 1126.2-, and 1524.6-keV γ rays have been assigned to the decay of excited states of 39 S, to date none have been placed within a level scheme. Binary grazing reactions with stable neutron-rich beams and heavy targets can be used to populate yrast and nearyrast states of moderately neutron-rich projectilelike species [5,13,[32][33][34] and, in general, experiments using such reactions, although unable to reach the most neutron-rich nuclear species currently accessible to experiment, provide more detailed spectroscopy than is currently possible using intermediate-energy Coulomb excitation, where the states that are populated are, in general, those that are connected directly to the ground state by E2 transitions [35]. Fusion-evaporation reactions with stable beams are unable to populate neutron-rich nuclei such as 39 S. Here, the yrast decay sequence of 39 S, populated in binary grazing reactions, has been studied.…”