Fig. 1
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Examples of the spectral fitting results for the AKARI/IRC rest frame 2.5-4.2 μm spectra of AGN-dominated and AGN-SF-composite galaxies. The top two rows show examples of the cases where the aliphatic hydrocarbon features are detected in the emission, while the bottom two rows show those detected in the absorption. A black line shows the total model spectrum, while red and blue lines correspond to the aromatic and aliphatic hydrocarbon features, respectively.
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