Review Article
Kilonova/Macronova Emission from Compact Binary Mergers
Figure 3
Expected observed spectra of the NS-NS merger model APR4-1215 () compared with the spectra of normal Type Ia SN 2005cf [60–62] and broad-line Type Ic SN 1998bw [63, 64]. The spectra are shown in AB magnitudes () at 200 Mpc distance. The corresponding absolute magnitudes are indicated in the right axis.