$\begin{figure}\par\includegraphics[width=8.85cm]{6895fig2.eps} \end{figure}$ Figure 2: True (solid) and observed (dashed) mass functions of four models. $\alpha _{\rm true}$ and $\alpha _{\rm obs}$ are given in the frames. The numbering refers to the model numbers given in Table 1.
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In the text

$\begin{figure}\par\includegraphics[width=8.2cm]{6895fig3.eps}\par\end{figure}$ Figure 3: The fraction of detected clouds for different true masses. x-axis is the mass in solar masses, y-axis is $N_{\rm detected}/N_{\rm total}$ .
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In the text

$\begin{figure}\par\includegraphics[width=6.7cm]{6895fig1.eps}\par\end{figure}$	Figure 1: An example of column density distribution for model number #1 (see Table 1).
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$\begin{figure}\par\includegraphics[width=8.85cm]{6895fig2.eps} \end{figure}$	Figure 2: True (solid) and observed (dashed) mass functions of four models. $\alpha _{\rm true}$ and $\alpha _{\rm obs}$ are given in the frames. The numbering refers to the model numbers given in Table 1.
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$\begin{figure}\par\includegraphics[width=8.2cm]{6895fig3.eps}\par\end{figure}$	Figure 3: The fraction of detected clouds for different true masses. x-axis is the mass in solar masses, y-axis is $N_{\rm detected}/N_{\rm total}$ .
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