“…The β − emitter 103 Ru can be produced by the irradiation of natural ruthenium ( nat Ru, composition: 96 Ru (5.54%), 98 Ru (1.87%), 99 Ru (12.76%), 100 Ru (12.60%), 101 Ru (17.06%), 102 Ru (31.55%), and 104 Ru (18.62%)) or of enriched 102 Ru with thermal neutrons via the 102 Ru(n, γ) 103 Ru reaction. 26,27 97 Ru can be produced by alpha particle induced nuclear reaction on natural molybdenum ( nat Mo) via nat Mo(α, xn) 97 Ru, 28,29 by the irradiation of enriched 96 Ru with thermal neutrons via the 96 Ru(n, γ) 97 Ru reaction or by proton irradiation of long-lived technetium-99 ( 99 Tc) via 99 Tc(p, 3n) 97 Ru reaction. 30 97 Ru decays by 100% electron capture, releasing photons with energies of 216 keV (86%) and 324 keV (11%), the former of which is within the energy window of clinical SPECT detectors.…”