Fig. 13
Total metal-to-dust ratios for GRB afterglows versus stellar mass of their host
galaxies. Black data are galaxies hosting a highly-extinguished afterglow using
the first values of Table 5, where the
three hosts with the highest 
are
labeled. The shaded area indicates the probability distribution for
optically-selected GRBs, represented by a log-normal distribution of
based on Schady et al. (2010) and a
Gaussian distribution in
log (M∗ [M⊙] ) based
on SGL09.
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