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Fig. 3.

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Bolometric and broadband light curves of the merger model. Several Ca-rich transient candidates are plotted as well for comparison: SN 2005E Perets et al. (2010), SN 2007ke, SN 2010et Kasliwal et al. (2012), and SN 2012hn Valenti et al. (2014). All data are taken from the Open Supernova Catalog (Guillochon et al. 2017).

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