logN(H I)/cm−2 + [X/H], as a function of Wr(λ 1560) (top panel), dust depletion, [X/Fe], (middle panel) and depletion-derived dust-to-gas ratio, κX, (bottom panel) for quasar and GRB absorbers with C I or H2 detections. The same symbols are used as in Fig. 11, but here we also include the GRB afterglows with non-detections of C I (marked by the dashed lines in the top panel and as black empty circles in the bottom panels).
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