Metallicity dependence of the CO-to-H2 and the [CI]-to-H2 conversion factors in galaxies

Open Access

Fig. 2

Input observed A_V-PDFs used in PDFCHEM. We used three different medians (m = 5 blue line, m = 10 green line, and m = 15 orange line) and three different widths (σ_PDF = 0.2 solid lines, σ_PDF = 0.4 dashed lines, and σ_PDF = 0.6 dotted lines) that corresponded to different values of the mean $\bar{A_{V,obs}}$ $\overline{A_{\text{V,obs}}}$ . Table 2 summarizes the properties of these distributions.

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