Fig. 3.
Bolometric LCs (top panel) and absolute V-band LCs (bottom panel) of SN 2017eaw and SN 2018aoq in comparison to well-studied SN 2004A, SN 2004et, SN 2005cs, SN 2008bk, SN 2012ec, and SN 2012aw. Absolute curves were computed using the distances and reddenings in Table 1 of MB19, except in the case of SN 2004et for which we use the new estimates of the distance (see text).
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