Image Details
Caption: Figure 29.
Ratio of Hα- and UV-based dust-uncorrected SFRs as a function of ﹩{E}_{\mathrm{star}}(B-V)﹩. The Hα-based SFRs are corrected for aperture loss. The solid line indicates the best-fit regression expressed by Equation (10) with ﹩{f}_{\mathrm{neb}}^{\mathrm{best}}=0.53\pm 0.01﹩. The dashed line indicates the relation with ﹩{f}_{\mathrm{neb}}=0.44﹩.
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