The relatively short-lived radionuclide 44 Ti is of considerable importance for the interpretation of nucleosynthesis in core collapse supernova environments. Production is predominantly through the 40 Ca(α,γ)44 Ti reaction, which has been studied in this work over the energy range Ecm = 2.73 -4.18 MeV, via direct γ counting and the 4π-summing technique, utilizing a previously characterized 12 inch × 12 inch single NaI crystal. The inferred reaction rate is compared here to both current experimental measurements and theoretical model calculations.