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The lightcurves have diverse sampling, diverse noise, generally a smooth behavior, with more variability at early times, rather than late times (after the $^{64}\mathrm{Ni}$ decay starts dominating).  Here is an example of a very good, very well sampled lightcurve, with photometry from 2 telescopes, which is not consistent within the tiny tiny errorbars: tiny, probably underestimated observational uncertainties: