Fig. 18.
Left panel: bolometric light curves, after (host + MW) extinction correction and K-correction. The solid lines are the best fits of the function also used to fit the r band. The systematic uncertainties in the distance (black segment) and in the bolometric correction (blue segment) are shown in the upper-right corner. Right panel: distribution of the absolute bolometric peak magnitudes for our sample. iPTF15eov and iPTF16asu are marked in blue. Blue vertical lines mark the average and the standard deviation of the distribution when including all of the objects. Red vertical lines mark the average and the standard deviation of the distribution when excluding iPTF15eov and iPTF16asu.
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