Bolometric light curves in the radioactive tail derived from the B and V-band photometry from EFOSC imaging, using the bolometric corrections of Pejcha & Prieto (2015a; PP15, blue dots) and Bersten & Hamuy (2009; MH09, green squares). The decay is faster than the expected from full trapping of ⁵⁶Co decay (showed as a dashed black line). The non-full trapping model from Clocchiatti & Wheeler (1997) gives a ⁵⁶Ni Mass of 0.0210  ±  0.0025 M_⊙ for the Pejcha & Prieto (2015a) bolometric corrections. The time scale for this fit is T₀ = 319 ± 33 days, which corresponds to a ejecta mass of 12 M_⊙ for an explosion energy of 1 foe.