Fig. 8
Top: a nebular spectrum of SN 2009E is compared with spectra of SNe 1998A (Pastorello et al. 2005) and 1987A (Pun et al. 1995) at a similar phase (~1 year). The nebular spectrum of SN 2009E was obtained averaging spectra of 2010 Jan. 22nd and 24th. Bottom: the nebular spectrum of SN 2009E is compared with spectra of underluminous type IIP SNe obtained about 1 year after core-collapse (Benetti et al. 2001; Pastorello et al. 2009).
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