Fig. 16
CO versus H2 column densities for the H2-bearing GRB-DLAs presented in this paper compared to the H2-bearing QSO-DLAs from Balashev et al. (2017); Noterdaeme et al. (2018); Ranjan et al. (2018). Additionally, we plot the results from Burgh et al. (2010) for sight-lines through diffuse and translucent clouds in the Galaxy and the result from Prochaska et al. (2009) for the DLA toward GRB 080607.
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