Fig. 5.
Binned rms residuals vs. bin size plot of the photometry of SN 2018gv on the second night. The rms of the binned residuals, rmsN, is shown as a black curve as a function of bin sizes. The grey error bars represent the uncertainty of rmsN. The red curve shows the expected rms σN and the saw-tooth shape of the black curve arises from the change in M.
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