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Fig. 4

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Spectral energy distribution of NGC 1313, together with the best-fit two-temperature modified blackbody plus PAH and stellar component model. The filled circles correspond to the integrated flux densities in the ten AKARI bands. The thick solid line shows the best-fit model. We indicate the warm dust (dotted line), cold dust (dash-dotted line), PAH (dashed line), and stellar (thin solid line) components.

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