Quantifying the informativity of emission lines to infer physical conditions in giant molecular clouds - I. Application to model predictions

Open Access

Fig. J.1

Line selection for G₀ in an environment similar to the Horsehead pillar, for the reference use case (reference integration time and no scaling factor, κ, in the observation simulator). The analysis is performed for different regimes of $A_{V}^{tot}$ $\[A_{V}^{\text {tot}}\]$ : all environments ( $3 \leq A_{V}^{tot} \leq 24$ $\[3 \leq A_{V}^{\text {tot }} \leq 24\]$ , panel a), translucent gas ( $3 \leq A_{V}^{tot} \leq 6$ $\[3 \leq A_{V}^{\text {tot }} \leq 6\]$ , panel b), filamentary gas ( $6 \leq A_{V}^{tot} \leq 12$ $\[6 \leq A_{V}^{\text {tot }} \leq 12\]$ , panel c), and dense cores ( $12 \leq A_{V}^{tot} \leq 24$ $\[12 \leq A_{V}^{\text {tot }} \leq 24\]$ , panel d). Orange bars correspond to [CI] and [CII] lines.

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