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Fig. 5

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Top: SED plots for A68/C0’s best stellar population fits using the two extinction laws. In the case of Calzetti, the fit including nebular emission was prefered. Bottom: global and FIR-only fits. The best fit for the full photometry uses a Seyfert galaxy template from P07 (shown in red) and an extra extinction of AV = 0.6 by the SMC law. The FIR only SED (in green) is by R09.

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