Vockenhuber, C.Ouellet, C OThe, L-SBuchmann, LCaggiano, JChen, A.A.D'Auria, J.M.Davids, B.Fogarty, LFrekers, D.Wallner, AntonVockenhuber, CRuiz, C.2015-12-130954-3899http://hdl.handle.net/1885/81906The nuclide 44Ti is predicted to be produced in significant quantities in core-collapse supernovae, and indeed it has been observed in the supernova remnant Cassiopeia-A by space-based γ-ray telescopes. The main production of 44Ti takes place in the α-r200810.1088/0954-3899/35/1/0140342015-12-11