Fig. 5
SFRUV-inclination relation shown in the top panels of Fig. 3, but with the attenuation curves of Tuffs et al. (2004) showing the expected change in flux, and hence SFRUV, with inclination. Green trends show the relations that best fit our data, with 
and 
for the local sample (left) and 
,
for the COSMOS sample (right). In the left panel, models shown have face-on B-band opacities of 
, 1.0, 2.0, 4.0, and 8.0 (from light to dark grey) and F = 0.22.
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