Image Details
Caption: Figure 10.
Comparisons of ﹩{f}_{\mathrm{esc}}^{\mathrm{MgII}}﹩ (in y-axes) with EW of Mg II λ2796 (top left), O32 (top right), and the internal extinction of the observed galaxy (bottom). In the bottom panel, the dashed lines represent expectations from dust extinction laws without resonant scattering (note that Calzetti et al. 2000 and Reddy et al. 2016a curves mostly overlap). Colors and labels are similar to Figure 9. See discussion in Section 4.2.
© 2022. The Author(s). Published by the American Astronomical Society.