Comparison between the I-band and ﹩{i}^{{\prime} }﹩-band light curves of SN 2012ec from C. Barbarino et al. (2015) and our late-time measurements. The ﹩{i}^{{\prime} }﹩-band magnitudes are subtracted by 0.5 to align with the I-band magnitudes. The Co-56 decay slope is also shown to illustrate the deviation of the observed flux from the expected radioactive decay.