Fig. 15.
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Comparison between the known double-peaked TDE spectra at various epochs and double-peaked AGN sources. The grey horizontal line denotes the continuum level for clarity in the top spectrum. Data for NGC 1097 are from Schimoia et al. (2015), for NGC 4958 from Ricci & Steiner (2019), for Arp 102B from Couto et al. (2013), for AT2018hyz from Short et al. (2020), and for PTF–09djl are from Arcavi et al. (2014).
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