Table 2: The parameter values of the precomputed KOSMA- $\tau$ PDR-model clumps are equidistant on logarithmic scale in steps of half an order of magnitude.
Quantity Parameter range

Density $n\ensuremath{_{\rm s}} / \ensuremath{{\rm cm}^{-3}}$ 10², ..., 10⁶

Mass $M\ensuremath{_{\rm cl}} / \ensuremath{{M}_{\rm\odot}}$ 10^-3, ..., 10³

FUV flux $\chi / {\ensuremath{\chi_{\rm D}} }$ 10⁰, ..., 10⁶

**Table 2:** The parameter values of the precomputed KOSMA- $\tau$ PDR-model clumps are equidistant on logarithmic scale in steps of half an order of magnitude.
Quantity	Parameter range
Density $n\ensuremath{_{\rm s}} / \ensuremath{{\rm cm}^{-3}}$	10², ..., 10⁶
Mass $M\ensuremath{_{\rm cl}} / \ensuremath{{M}_{\rm\odot}}$	10^-3, ..., 10³
FUV flux $\chi / {\ensuremath{\chi_{\rm D}} }$	10⁰, ..., 10⁶

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