Image Details
Caption: Figure 4.
Left panels: the same as in Figure 3, but comparing the rest-frame BVi-band light curves of KSN-2016M to the best-fit power-law + Gaussian model (dashed curves; Equations D1 + D2) with ﹩{\chi }_{{\rm{R}}}^{2}﹩ = 1.1 and its power-law component (solid curves). Right panels: comparison of the residuals of the power-law + Gaussian (open circles) to those of its power-law component (filled circles).
© 2025. The Author(s). Published by the American Astronomical Society.