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Fig. 6.

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Optical/UV SED model adopted for this study (a) without absorption, for different values of kTmax (dash-dotted lines), keeping Kuvo constant at 2 × 105, and for different values of Kuvo (dashed lines), keeping kTmax constant at 2.7 eV and (b) with absorption, for different values of E(B − V)HG, with kTmax = 2.7 eV, Kuvo = 2 × 105, and E(B − V)MW = 0.05. The former plot shows possible degeneracy between parameters kTmax and Kuvo, while the latter shows effects of host galaxy dust extinction on the optical/UV SED model, almost negligible for E(B − V)HG ≤ 0.01.

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