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Fig. 9
ETGs with a hot dust continuum. We classify such MIR ETG spectra as Class-4. H2 molecular lines, PAH 7.6 μm, 11.3 μm, 12.7 μm and 17 μm complexes and ionic line positions are indicated at the top of the spectrum. NGC 1052 is a prototypical LINER while IC 5063 is an ETG with a Seyfert nucleus.
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