Pseudo-bolometric light curves of a handful of well-observed LRNe from Tylenda (2005), Tylenda et al. (2011), Williams et al. (2015), Cai et al. (2019), and Pastorello et al. (2019a), plotted along with that of AT 2014ej. The solid red line extended beyond the UVOIR light curve of AT 2014ej corresponds to CHASE unfiltered photometry. Two LRN models published by Metzger & Pejcha (2017) are also overplotted as gray lines. This includes the light curve computed for theirY fiducial model assuming a binary mass of 10 M_⊙, a semimajor axis of a = 30 R_⊙, and a predynamical mass runaway time of t_run = 10 ⋅ t_dyn, as well as a second more luminous light curve produced from a model assuming a higher binary mass of 30 M_⊙.